|
| Errata: Photometry Net, Flux (PFLX) Files |
Note that for this table there are several entries per source data file. The Line value below refers to the line number in that table.
Filename CDROM Path Type Line Comments
------------------------------------------------------------------------------------------------------
pflx0001 HAL_0019 /y1985/m08/d24 table 1 Used PHOTOM* to recalc X's, k's calc'd from
HD3379, used k's to calc dM for each star entry,
mean and sdev to get dM and error (dM), error
(k) adopted as 0.01
pflx0001 HAL_0019 /y1985/m08/d24 table 2 Used PHOTOM* to recalc X's, k's calc'd from
HD3379, used k's to calc dM for each star entry,
mean and sdev to get dM and error (dM), error
(k) adopted as 0.01
pflx0001 HAL_0019 /y1985/m08/d24 table 3 Used PHOTOM* to recalc X's, k's calc'd from
HD3379, used k's to calc dM for each star entry,
mean and sdev to get dM and error (dM), error
(k) adopted as 0.01
pflx0001 HAL_0019 /y1985/m08/d24 table 4 Used PHOTOM* to recalc X's, k's calc'd from
HD3379, used k's to calc dM for each star entry,
mean and sdev to get dM and error (dM), error
(k) adopted as 0.01
pflx0001 HAL_0019 /y1985/m08/d24 table 5 Used PHOTOM* to recalc X's, k's calc'd from
HD3379, used k's to calc dM for each star entry,
mean and sdev to get dM and error (dM), error
(k) adopted as 0.01
pflx0002 HAL_0019 /y1985/m08/d26 table 6 Used PHOTOM* to recalc X's, k's calc'd from
HD3379, used k's to calc dM for each star entry,
mean and sdev to get dM and error (dM), error
(k) adopted as 0.01
pflx0002 HAL_0019 /y1985/m08/d26 table 7 Used PHOTOM* to recalc X's, k's calc'd from
HD3379, used k's to calc dM for each star entry,
mean and sdev to get dM and error (dM), error
(k) adopted as 0.01
pflx0002 HAL_0019 /y1985/m08/d26 table 8 Used PHOTOM* to recalc X's, k's calc'd from
HD3379, used k's to calc dM for each star entry,
mean and sdev to get dM and error (dM), error
(k) adopted as 0.01
pflx0002 HAL_0019 /y1985/m08/d26 table 9 Used PHOTOM* to recalc X's, k's calc'd from
HD3379, used k's to calc dM for each star entry,
mean and sdev to get dM and error (dM), error
(k) adopted as 0.01
pflx0002 HAL_0019 /y1985/m08/d26 table 10 Used PHOTOM* to recalc X's, k's calc'd from
HD3379, used k's to calc dM for each star entry,
mean and sdev to get dM and error (dM), error
(k) adopted as 0.01
pflx0002 HAL_0019 /y1985/m08/d26 table 11 Used PHOTOM* to recalc X's, k's calc'd from
HD3379, used k's to calc dM for each star entry,
mean and sdev to get dM and error (dM), error
(k) adopted as 0.01
pflx0004 HAL_0019 /y1985/m09/d09 table 16 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0004 HAL_0019 /y1985/m09/d09 table 17 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0004 HAL_0019 /y1985/m09/d09 table 18 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0004 HAL_0019 /y1985/m09/d09 table 19 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0004 HAL_0019 /y1985/m09/d09 table 20 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0004 HAL_0019 /y1985/m09/d09 table 21 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0005 HAL_0019 /y1985/m09/d10 table 22 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0005 HAL_0019 /y1985/m09/d10 table 23 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0005 HAL_0019 /y1985/m09/d10 table 24 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0005 HAL_0019 /y1985/m09/d10 table 25 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0005 HAL_0019 /y1985/m09/d10 table 26 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0005 HAL_0019 /y1985/m09/d10 table 27 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0005 HAL_0019 /y1985/m09/d10 table 28 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0005 HAL_0019 /y1985/m09/d10 table 29 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0006 HAL_0019 /y1985/m09/d10 table 30 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0006 HAL_0019 /y1985/m09/d10 table 31 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0006 HAL_0019 /y1985/m09/d10 table 32 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0006 HAL_0019 /y1985/m09/d10 table 33 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0006 HAL_0019 /y1985/m09/d10 table 34 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0006 HAL_0019 /y1985/m09/d10 table 35 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0006 HAL_0019 /y1985/m09/d10 table 36 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0006 HAL_0019 /y1985/m09/d10 table 37 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0007 HAL_0019 /y1985/m09/d10 table 38 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0008 HAL_0019 /y1985/m09/d11 table 39 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0008 HAL_0019 /y1985/m09/d11 table 40 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0008 HAL_0019 /y1985/m09/d11 table 41 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0008 HAL_0019 /y1985/m09/d11 table 42 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0008 HAL_0019 /y1985/m09/d11 table 43 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0008 HAL_0019 /y1985/m09/d11 table 44 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0008 HAL_0019 /y1985/m09/d11 table 45 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0008 HAL_0019 /y1985/m09/d11 table 46 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0009 HAL_0019 /y1985/m09/d11 table 47 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0009 HAL_0019 /y1985/m09/d11 table 48 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0009 HAL_0019 /y1985/m09/d11 table 49 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0009 HAL_0019 /y1985/m09/d11 table 50 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0009 HAL_0019 /y1985/m09/d11 table 51 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0009 HAL_0019 /y1985/m09/d11 table 52 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0009 HAL_0019 /y1985/m09/d11 table 53 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0009 HAL_0019 /y1985/m09/d11 table 54 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0010 HAL_0019 /y1985/m09/d11 table 55 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0011 HAL_0019 /y1985/m09/d14 table 56 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0011 HAL_0019 /y1985/m09/d14 table 57 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0011 HAL_0019 /y1985/m09/d14 table 58 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0011 HAL_0019 /y1985/m09/d14 table 59 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0011 HAL_0019 /y1985/m09/d14 table 60 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0011 HAL_0019 /y1985/m09/d14 table 61 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0011 HAL_0019 /y1985/m09/d14 table 62 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0011 HAL_0019 /y1985/m09/d14 table 63 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0012 HAL_0019 /y1985/m09/d14 table 64 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0012 HAL_0019 /y1985/m09/d14 table 65 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0012 HAL_0019 /y1985/m09/d14 table 66 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0012 HAL_0019 /y1985/m09/d14 table 67 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0012 HAL_0019 /y1985/m09/d14 table 68 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0012 HAL_0019 /y1985/m09/d14 table 69 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0012 HAL_0019 /y1985/m09/d14 table 70 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0012 HAL_0019 /y1985/m09/d14 table 71 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0013 HAL_0019 /y1985/m09/d14 table 72 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0013 HAL_0019 /y1985/m09/d14 table 73 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0013 HAL_0019 /y1985/m09/d14 table 74 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0013 HAL_0019 /y1985/m09/d14 table 75 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0013 HAL_0019 /y1985/m09/d14 table 76 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0013 HAL_0019 /y1985/m09/d14 table 77 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0013 HAL_0019 /y1985/m09/d14 table 78 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0013 HAL_0019 /y1985/m09/d14 table 79 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0014 HAL_0019 /y1985/m09/d14 table 80 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0014 HAL_0019 /y1985/m09/d14 table 81 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0014 HAL_0019 /y1985/m09/d14 table 82 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0014 HAL_0019 /y1985/m09/d14 table 83 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0014 HAL_0019 /y1985/m09/d14 table 84 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0014 HAL_0019 /y1985/m09/d14 table 85 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0014 HAL_0019 /y1985/m09/d14 table 86 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0014 HAL_0019 /y1985/m09/d14 table 87 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0015 HAL_0019 /y1985/m09/d15 table 88 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0015 HAL_0019 /y1985/m09/d15 table 89 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0015 HAL_0019 /y1985/m09/d15 table 90 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0015 HAL_0019 /y1985/m09/d15 table 91 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0015 HAL_0019 /y1985/m09/d15 table 92 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0015 HAL_0019 /y1985/m09/d15 table 93 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0015 HAL_0019 /y1985/m09/d15 table 94 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0015 HAL_0019 /y1985/m09/d15 table 95 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0016 HAL_0019 /y1985/m09/d15 table 96 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0016 HAL_0019 /y1985/m09/d15 table 97 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0016 HAL_0019 /y1985/m09/d15 table 98 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0016 HAL_0019 /y1985/m09/d15 table 99 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0016 HAL_0019 /y1985/m09/d15 table 100 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0016 HAL_0019 /y1985/m09/d15 table 101 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0016 HAL_0019 /y1985/m09/d15 table 102 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0016 HAL_0019 /y1985/m09/d15 table 103 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0017 HAL_0019 /y1985/m09/d15 table 104 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0017 HAL_0019 /y1985/m09/d15 table 105 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0017 HAL_0019 /y1985/m09/d15 table 106 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0017 HAL_0019 /y1985/m09/d15 table 107 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0017 HAL_0019 /y1985/m09/d15 table 108 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0017 HAL_0019 /y1985/m09/d15 table 109 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0017 HAL_0019 /y1985/m09/d15 table 110 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0017 HAL_0019 /y1985/m09/d15 table 111 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0018 HAL_0019 /y1985/m09/d15 table 112 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0018 HAL_0019 /y1985/m09/d15 table 113 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0018 HAL_0019 /y1985/m09/d15 table 114 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0018 HAL_0019 /y1985/m09/d15 table 115 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0018 HAL_0019 /y1985/m09/d15 table 116 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0018 HAL_0019 /y1985/m09/d15 table 117 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0018 HAL_0019 /y1985/m09/d15 table 118 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0018 HAL_0019 /y1985/m09/d15 table 119 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0021 HAL_0019 /y1985/m09/d16 table 136 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0021 HAL_0019 /y1985/m09/d16 table 137 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0021 HAL_0019 /y1985/m09/d16 table 138 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0021 HAL_0019 /y1985/m09/d16 table 139 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0021 HAL_0019 /y1985/m09/d16 table 140 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0021 HAL_0019 /y1985/m09/d16 table 141 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0021 HAL_0019 /y1985/m09/d16 table 142 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0021 HAL_0019 /y1985/m09/d16 table 143 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0022 HAL_0019 /y1985/m09/d16 table 144 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0022 HAL_0019 /y1985/m09/d16 table 145 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0022 HAL_0019 /y1985/m09/d16 table 146 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0022 HAL_0019 /y1985/m09/d16 table 147 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0022 HAL_0019 /y1985/m09/d16 table 148 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0022 HAL_0019 /y1985/m09/d16 table 149 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0022 HAL_0019 /y1985/m09/d16 table 150 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0022 HAL_0019 /y1985/m09/d16 table 151 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0023 HAL_0019 /y1985/m09/d16 table 152 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0023 HAL_0019 /y1985/m09/d16 table 153 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0023 HAL_0019 /y1985/m09/d16 table 154 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0023 HAL_0019 /y1985/m09/d16 table 155 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0023 HAL_0019 /y1985/m09/d16 table 156 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0023 HAL_0019 /y1985/m09/d16 table 157 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0023 HAL_0019 /y1985/m09/d16 table 158 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0023 HAL_0019 /y1985/m09/d16 table 159 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0024 HAL_0019 /y1985/m09/d16 table 160 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0024 HAL_0019 /y1985/m09/d16 table 161 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0024 HAL_0019 /y1985/m09/d16 table 162 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0024 HAL_0019 /y1985/m09/d16 table 163 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0024 HAL_0019 /y1985/m09/d16 table 164 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0024 HAL_0019 /y1985/m09/d16 table 165 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0024 HAL_0019 /y1985/m09/d16 table 166 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0024 HAL_0019 /y1985/m09/d16 table 167 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0025 HAL_0019 /y1985/m09/d16 table 168 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0025 HAL_0019 /y1985/m09/d16 table 169 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0025 HAL_0019 /y1985/m09/d16 table 170 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0025 HAL_0019 /y1985/m09/d16 table 171 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0028 HAL_0019 /y1985/m09/d18 table 188 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0028 HAL_0019 /y1985/m09/d18 table 189 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0028 HAL_0019 /y1985/m09/d18 table 190 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0028 HAL_0019 /y1985/m09/d18 table 191 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0028 HAL_0019 /y1985/m09/d18 table 192 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0028 HAL_0019 /y1985/m09/d18 table 193 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0028 HAL_0019 /y1985/m09/d18 table 194 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0028 HAL_0019 /y1985/m09/d18 table 195 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0029 HAL_0019 /y1985/m09/d18 table 196 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0029 HAL_0019 /y1985/m09/d18 table 197 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0029 HAL_0019 /y1985/m09/d18 table 198 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0029 HAL_0019 /y1985/m09/d18 table 199 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0029 HAL_0019 /y1985/m09/d18 table 200 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0029 HAL_0019 /y1985/m09/d18 table 201 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0029 HAL_0019 /y1985/m09/d18 table 202 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0029 HAL_0019 /y1985/m09/d18 table 203 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0030 HAL_0019 /y1985/m09/d18 table 204 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0030 HAL_0019 /y1985/m09/d18 table 205 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0030 HAL_0019 /y1985/m09/d18 table 206 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0030 HAL_0019 /y1985/m09/d18 table 207 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0030 HAL_0019 /y1985/m09/d18 table 208 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0030 HAL_0019 /y1985/m09/d18 table 209 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0030 HAL_0019 /y1985/m09/d18 table 210 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0030 HAL_0019 /y1985/m09/d18 table 211 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0031 HAL_0019 /y1985/m09/d18 table 212 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0031 HAL_0019 /y1985/m09/d18 table 213 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0031 HAL_0019 /y1985/m09/d18 table 214 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0031 HAL_0019 /y1985/m09/d18 table 215 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0031 HAL_0019 /y1985/m09/d18 table 216 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0031 HAL_0019 /y1985/m09/d18 table 217 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0031 HAL_0019 /y1985/m09/d18 table 218 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0031 HAL_0019 /y1985/m09/d18 table 219 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0032 HAL_0019 /y1985/m09/d18 table 220 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0032 HAL_0019 /y1985/m09/d18 table 221 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0032 HAL_0019 /y1985/m09/d18 table 222 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0032 HAL_0019 /y1985/m09/d18 table 223 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0032 HAL_0019 /y1985/m09/d18 table 224 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0032 HAL_0019 /y1985/m09/d18 table 225 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0032 HAL_0019 /y1985/m09/d18 table 226 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0032 HAL_0019 /y1985/m09/d18 table 227 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0033 HAL_0019 /y1985/m09/d19 table 228 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0033 HAL_0019 /y1985/m09/d19 table 229 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0033 HAL_0019 /y1985/m09/d19 table 230 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0033 HAL_0019 /y1985/m09/d19 table 231 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0033 HAL_0019 /y1985/m09/d19 table 232 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0033 HAL_0019 /y1985/m09/d19 table 233 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0033 HAL_0019 /y1985/m09/d19 table 234 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0034 HAL_0019 /y1985/m09/d20 table 235 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0034 HAL_0019 /y1985/m09/d20 table 236 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0034 HAL_0019 /y1985/m09/d20 table 237 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0034 HAL_0019 /y1985/m09/d20 table 238 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0034 HAL_0019 /y1985/m09/d20 table 239 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0034 HAL_0019 /y1985/m09/d20 table 240 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0034 HAL_0019 /y1985/m09/d20 table 241 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0034 HAL_0019 /y1985/m09/d20 table 242 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0035 HAL_0019 /y1985/m09/d20 table 243 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0035 HAL_0019 /y1985/m09/d20 table 244 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0035 HAL_0019 /y1985/m09/d20 table 245 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0035 HAL_0019 /y1985/m09/d20 table 246 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0035 HAL_0019 /y1985/m09/d20 table 247 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0035 HAL_0019 /y1985/m09/d20 table 248 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0035 HAL_0019 /y1985/m09/d20 table 249 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0035 HAL_0019 /y1985/m09/d20 table 250 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0036 HAL_0019 /y1985/m09/d20 table 251 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0036 HAL_0019 /y1985/m09/d20 table 252 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0036 HAL_0019 /y1985/m09/d20 table 253 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0036 HAL_0019 /y1985/m09/d20 table 254 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0036 HAL_0019 /y1985/m09/d20 table 255 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0036 HAL_0019 /y1985/m09/d20 table 256 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0036 HAL_0019 /y1985/m09/d20 table 257 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0036 HAL_0019 /y1985/m09/d20 table 258 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0037 HAL_0019 /y1985/m09/d20 table 259 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0037 HAL_0019 /y1985/m09/d20 table 260 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0037 HAL_0019 /y1985/m09/d20 table 261 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0037 HAL_0019 /y1985/m09/d20 table 262 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0037 HAL_0019 /y1985/m09/d20 table 263 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0037 HAL_0019 /y1985/m09/d20 table 264 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0037 HAL_0019 /y1985/m09/d20 table 265 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0037 HAL_0019 /y1985/m09/d20 table 266 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0038 HAL_0019 /y1985/m09/d20 table 267 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0038 HAL_0019 /y1985/m09/d20 table 268 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0038 HAL_0019 /y1985/m09/d20 table 269 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0038 HAL_0019 /y1985/m09/d20 table 270 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0038 HAL_0019 /y1985/m09/d20 table 271 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0038 HAL_0019 /y1985/m09/d20 table 272 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0038 HAL_0019 /y1985/m09/d20 table 273 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0038 HAL_0019 /y1985/m09/d20 table 274 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0039 HAL_0019 /y1985/m09/d20 table 275 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0039 HAL_0019 /y1985/m09/d20 table 276 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0039 HAL_0019 /y1985/m09/d20 table 277 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0039 HAL_0019 /y1985/m09/d20 table 278 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0039 HAL_0019 /y1985/m09/d20 table 279 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0039 HAL_0019 /y1985/m09/d20 table 280 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0039 HAL_0019 /y1985/m09/d20 table 281 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0039 HAL_0019 /y1985/m09/d20 table 282 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0040 HAL_0019 /y1985/m09/d20 table 283 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0040 HAL_0019 /y1985/m09/d20 table 284 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0040 HAL_0019 /y1985/m09/d20 table 285 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0040 HAL_0019 /y1985/m09/d20 table 286 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0040 HAL_0019 /y1985/m09/d20 table 287 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0040 HAL_0019 /y1985/m09/d20 table 288 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0040 HAL_0019 /y1985/m09/d20 table 289 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0040 HAL_0019 /y1985/m09/d20 table 290 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0041 HAL_0019 /y1985/m09/d21 table 291 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0041 HAL_0019 /y1985/m09/d21 table 292 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0041 HAL_0019 /y1985/m09/d21 table 293 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0041 HAL_0019 /y1985/m09/d21 table 294 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0041 HAL_0019 /y1985/m09/d21 table 295 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0041 HAL_0019 /y1985/m09/d21 table 296 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0041 HAL_0019 /y1985/m09/d21 table 297 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0041 HAL_0019 /y1985/m09/d21 table 298 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0049 HAL_0019 /y1985/m09/d22 table 349 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0049 HAL_0019 /y1985/m09/d22 table 350 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0049 HAL_0019 /y1985/m09/d22 table 351 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0049 HAL_0019 /y1985/m09/d22 table 352 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0049 HAL_0019 /y1985/m09/d22 table 353 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0049 HAL_0019 /y1985/m09/d22 table 354 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0049 HAL_0019 /y1985/m09/d22 table 355 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0049 HAL_0019 /y1985/m09/d22 table 356 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0050 HAL_0019 /y1985/m09/d22 table 357 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0050 HAL_0019 /y1985/m09/d22 table 358 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0050 HAL_0019 /y1985/m09/d22 table 359 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0050 HAL_0019 /y1985/m09/d22 table 360 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0050 HAL_0019 /y1985/m09/d22 table 361 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0050 HAL_0019 /y1985/m09/d22 table 362 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0050 HAL_0019 /y1985/m09/d22 table 363 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0050 HAL_0019 /y1985/m09/d22 table 364 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0051 HAL_0019 /y1985/m09/d22 table 365 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0051 HAL_0019 /y1985/m09/d22 table 366 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0051 HAL_0019 /y1985/m09/d22 table 367 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0051 HAL_0019 /y1985/m09/d22 table 368 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0051 HAL_0019 /y1985/m09/d22 table 369 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0051 HAL_0019 /y1985/m09/d22 table 370 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0051 HAL_0019 /y1985/m09/d22 table 371 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0051 HAL_0019 /y1985/m09/d22 table 372 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0052 HAL_0019 /y1985/m09/d22 table 373 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0052 HAL_0019 /y1985/m09/d22 table 374 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0052 HAL_0019 /y1985/m09/d22 table 375 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0052 HAL_0019 /y1985/m09/d22 table 376 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0052 HAL_0019 /y1985/m09/d22 table 377 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0052 HAL_0019 /y1985/m09/d22 table 378 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0052 HAL_0019 /y1985/m09/d22 table 379 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0052 HAL_0019 /y1985/m09/d22 table 380 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0053 HAL_0019 /y1985/m09/d22 table 381 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0053 HAL_0019 /y1985/m09/d22 table 382 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0053 HAL_0019 /y1985/m09/d22 table 383 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0053 HAL_0019 /y1985/m09/d22 table 384 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0053 HAL_0019 /y1985/m09/d22 table 385 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0053 HAL_0019 /y1985/m09/d22 table 386 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0053 HAL_0019 /y1985/m09/d22 table 387 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0053 HAL_0019 /y1985/m09/d22 table 388 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0054 HAL_0019 /y1985/m09/d22 table 389 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0054 HAL_0019 /y1985/m09/d22 table 390 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0054 HAL_0019 /y1985/m09/d22 table 391 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0054 HAL_0019 /y1985/m09/d22 table 392 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0054 HAL_0019 /y1985/m09/d22 table 393 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0054 HAL_0019 /y1985/m09/d22 table 394 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0054 HAL_0019 /y1985/m09/d22 table 395 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0054 HAL_0019 /y1985/m09/d22 table 396 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0055 HAL_0019 /y1985/m09/d22 table 397 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0055 HAL_0019 /y1985/m09/d22 table 398 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0055 HAL_0019 /y1985/m09/d22 table 399 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0055 HAL_0019 /y1985/m09/d22 table 400 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0055 HAL_0019 /y1985/m09/d22 table 401 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0055 HAL_0019 /y1985/m09/d22 table 402 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0055 HAL_0019 /y1985/m09/d22 table 403 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0055 HAL_0019 /y1985/m09/d22 table 404 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0056 HAL_0019 /y1985/m09/d22 table 405 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0056 HAL_0019 /y1985/m09/d22 table 406 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0056 HAL_0019 /y1985/m09/d22 table 407 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0056 HAL_0019 /y1985/m09/d22 table 408 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0056 HAL_0019 /y1985/m09/d22 table 409 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0056 HAL_0019 /y1985/m09/d22 table 410 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0056 HAL_0019 /y1985/m09/d22 table 411 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0056 HAL_0019 /y1985/m09/d22 table 412 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0066 HAL_0019 /y1985/m09/d24/h18 table 475 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0066 HAL_0019 /y1985/m09/d24/h18 table 476 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0066 HAL_0019 /y1985/m09/d24/h18 table 477 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0066 HAL_0019 /y1985/m09/d24/h18 table 478 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0066 HAL_0019 /y1985/m09/d24/h18 table 479 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0066 HAL_0019 /y1985/m09/d24/h18 table 480 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0066 HAL_0019 /y1985/m09/d24/h18 table 481 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0066 HAL_0019 /y1985/m09/d24/h18 table 482 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0067 HAL_0019 /y1985/m09/d24/h18 table 483 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0067 HAL_0019 /y1985/m09/d24/h18 table 484 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0067 HAL_0019 /y1985/m09/d24/h18 table 485 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0067 HAL_0019 /y1985/m09/d24/h18 table 486 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0067 HAL_0019 /y1985/m09/d24/h18 table 487 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0067 HAL_0019 /y1985/m09/d24/h18 table 488 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0067 HAL_0019 /y1985/m09/d24/h18 table 489 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0067 HAL_0019 /y1985/m09/d24/h18 table 490 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0068 HAL_0019 /y1985/m09/d24/h18 table 491 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0068 HAL_0019 /y1985/m09/d24/h18 table 492 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0068 HAL_0019 /y1985/m09/d24/h18 table 493 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0068 HAL_0019 /y1985/m09/d24/h18 table 494 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0068 HAL_0019 /y1985/m09/d24/h18 table 495 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0068 HAL_0019 /y1985/m09/d24/h18 table 496 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0068 HAL_0019 /y1985/m09/d24/h18 table 497 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0068 HAL_0019 /y1985/m09/d24/h18 table 498 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0069 HAL_0019 /y1985/m09/d24/h18 table 499 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0069 HAL_0019 /y1985/m09/d24/h18 table 500 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0069 HAL_0019 /y1985/m09/d24/h18 table 501 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0069 HAL_0019 /y1985/m09/d24/h18 table 502 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0069 HAL_0019 /y1985/m09/d24/h18 table 503 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0069 HAL_0019 /y1985/m09/d24/h18 table 504 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0069 HAL_0019 /y1985/m09/d24/h18 table 505 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0069 HAL_0019 /y1985/m09/d24/h18 table 506 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0070 HAL_0019 /y1985/m09/d24/h18 table 507 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0070 HAL_0019 /y1985/m09/d24/h18 table 508 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0070 HAL_0019 /y1985/m09/d24/h18 table 509 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0070 HAL_0019 /y1985/m09/d24/h18 table 510 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0070 HAL_0019 /y1985/m09/d24/h18 table 511 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0070 HAL_0019 /y1985/m09/d24/h18 table 512 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0070 HAL_0019 /y1985/m09/d24/h18 table 513 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0070 HAL_0019 /y1985/m09/d24/h18 table 514 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0071 HAL_0019 /y1985/m09/d24/h18 table 515 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0071 HAL_0019 /y1985/m09/d24/h18 table 516 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0071 HAL_0019 /y1985/m09/d24/h18 table 517 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0071 HAL_0019 /y1985/m09/d24/h18 table 518 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0071 HAL_0019 /y1985/m09/d24/h18 table 519 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0071 HAL_0019 /y1985/m09/d24/h18 table 520 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0071 HAL_0019 /y1985/m09/d24/h18 table 521 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0071 HAL_0019 /y1985/m09/d24/h18 table 522 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0072 HAL_0019 /y1985/m09/d24/h18 table 523 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0072 HAL_0019 /y1985/m09/d24/h18 table 524 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0072 HAL_0019 /y1985/m09/d24/h18 table 525 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0073 HAL_0019 /y1985/m09/d25 table 526 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0073 HAL_0019 /y1985/m09/d25 table 527 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0073 HAL_0019 /y1985/m09/d25 table 528 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0073 HAL_0019 /y1985/m09/d25 table 529 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0073 HAL_0019 /y1985/m09/d25 table 530 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0073 HAL_0019 /y1985/m09/d25 table 531 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0073 HAL_0019 /y1985/m09/d25 table 532 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0073 HAL_0019 /y1985/m09/d25 table 533 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0074 HAL_0019 /y1985/m09/d25 table 534 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0074 HAL_0019 /y1985/m09/d25 table 535 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0074 HAL_0019 /y1985/m09/d25 table 536 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0074 HAL_0019 /y1985/m09/d25 table 537 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0074 HAL_0019 /y1985/m09/d25 table 538 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0074 HAL_0019 /y1985/m09/d25 table 539 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0074 HAL_0019 /y1985/m09/d25 table 540 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0074 HAL_0019 /y1985/m09/d25 table 541 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0075 HAL_0019 /y1985/m09/d25 table 542 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0075 HAL_0019 /y1985/m09/d25 table 543 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0075 HAL_0019 /y1985/m09/d25 table 544 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0075 HAL_0019 /y1985/m09/d25 table 545 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0075 HAL_0019 /y1985/m09/d25 table 546 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0075 HAL_0019 /y1985/m09/d25 table 547 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0075 HAL_0019 /y1985/m09/d25 table 548 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0075 HAL_0019 /y1985/m09/d25 table 549 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0076 HAL_0019 /y1985/m09/d25 table 550 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0076 HAL_0019 /y1985/m09/d25 table 551 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0076 HAL_0019 /y1985/m09/d25 table 552 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0076 HAL_0019 /y1985/m09/d25 table 553 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0076 HAL_0019 /y1985/m09/d25 table 554 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0076 HAL_0019 /y1985/m09/d25 table 555 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0076 HAL_0019 /y1985/m09/d25 table 556 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0076 HAL_0019 /y1985/m09/d25 table 557 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0077 HAL_0019 /y1985/m09/d25 table 558 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0077 HAL_0019 /y1985/m09/d25 table 559 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0077 HAL_0019 /y1985/m09/d25 table 560 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0077 HAL_0019 /y1985/m09/d25 table 561 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0077 HAL_0019 /y1985/m09/d25 table 562 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0077 HAL_0019 /y1985/m09/d25 table 563 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0077 HAL_0019 /y1985/m09/d25 table 564 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0077 HAL_0019 /y1985/m09/d25 table 565 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0087 HAL_0019 /y1985/m10/d17 table 643 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0087 HAL_0019 /y1985/m10/d17 table 644 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0087 HAL_0019 /y1985/m10/d17 table 645 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0087 HAL_0019 /y1985/m10/d17 table 646 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0087 HAL_0019 /y1985/m10/d17 table 647 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0087 HAL_0019 /y1985/m10/d17 table 648 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0087 HAL_0019 /y1985/m10/d17 table 649 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0087 HAL_0019 /y1985/m10/d17 table 650 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0088 HAL_0019 /y1985/m10/d17 table 651 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0088 HAL_0019 /y1985/m10/d17 table 652 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0088 HAL_0019 /y1985/m10/d17 table 653 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0088 HAL_0019 /y1985/m10/d17 table 654 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0088 HAL_0019 /y1985/m10/d17 table 655 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0088 HAL_0019 /y1985/m10/d17 table 656 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0088 HAL_0019 /y1985/m10/d17 table 657 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0088 HAL_0019 /y1985/m10/d17 table 658 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0089 HAL_0019 /y1985/m10/d17 table 659 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0089 HAL_0019 /y1985/m10/d17 table 660 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0089 HAL_0019 /y1985/m10/d17 table 661 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0089 HAL_0019 /y1985/m10/d17 table 662 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0089 HAL_0019 /y1985/m10/d17 table 663 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0089 HAL_0019 /y1985/m10/d17 table 664 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0090 HAL_0019 /y1985/m10/d17 table 665 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0090 HAL_0019 /y1985/m10/d17 table 666 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0090 HAL_0019 /y1985/m10/d17 table 667 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0090 HAL_0019 /y1985/m10/d17 table 668 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0090 HAL_0019 /y1985/m10/d17 table 669 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0090 HAL_0019 /y1985/m10/d17 table 670 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0090 HAL_0019 /y1985/m10/d17 table 671 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0090 HAL_0019 /y1985/m10/d17 table 672 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0091 HAL_0019 /y1985/m10/d18 table 673 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0091 HAL_0019 /y1985/m10/d18 table 674 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0091 HAL_0019 /y1985/m10/d18 table 675 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0091 HAL_0019 /y1985/m10/d18 table 676 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0091 HAL_0019 /y1985/m10/d18 table 677 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0091 HAL_0019 /y1985/m10/d18 table 678 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0091 HAL_0019 /y1985/m10/d18 table 679 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0091 HAL_0019 /y1985/m10/d18 table 680 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0092 HAL_0019 /y1985/m10/d18 table 681 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0092 HAL_0019 /y1985/m10/d18 table 682 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0092 HAL_0019 /y1985/m10/d18 table 683 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0092 HAL_0019 /y1985/m10/d18 table 684 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0092 HAL_0019 /y1985/m10/d18 table 685 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0092 HAL_0019 /y1985/m10/d18 table 686 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0092 HAL_0019 /y1985/m10/d18 table 687 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0092 HAL_0019 /y1985/m10/d18 table 688 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0093 HAL_0019 /y1985/m10/d19 table 689 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0093 HAL_0019 /y1985/m10/d19 table 690 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0093 HAL_0019 /y1985/m10/d19 table 691 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0093 HAL_0019 /y1985/m10/d19 table 692 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0093 HAL_0019 /y1985/m10/d19 table 693 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0093 HAL_0019 /y1985/m10/d19 table 694 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0093 HAL_0019 /y1985/m10/d19 table 695 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0093 HAL_0019 /y1985/m10/d19 table 696 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0094 HAL_0019 /y1985/m10/d19 table 697 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0094 HAL_0019 /y1985/m10/d19 table 698 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0094 HAL_0019 /y1985/m10/d19 table 699 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0094 HAL_0019 /y1985/m10/d19 table 700 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0094 HAL_0019 /y1985/m10/d19 table 701 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0094 HAL_0019 /y1985/m10/d19 table 702 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0094 HAL_0019 /y1985/m10/d19 table 703 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0094 HAL_0019 /y1985/m10/d19 table 704 Used k's from 10/20/85, 51020, added INTERP1**
dM's as X=0 Mi-Ms star entries, then calculated
dM's and error (dM) from mean and sdev, unknown
error (k) absorbed into error (dM)
pflx0097 HAL_0019 /y1985/m10/d20 table 721 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0097 HAL_0019 /y1985/m10/d20 table 722 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0097 HAL_0019 /y1985/m10/d20 table 723 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0097 HAL_0019 /y1985/m10/d20 table 724 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0097 HAL_0019 /y1985/m10/d20 table 725 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0097 HAL_0019 /y1985/m10/d20 table 726 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0097 HAL_0019 /y1985/m10/d20 table 727 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0097 HAL_0019 /y1985/m10/d20 table 728 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0098 HAL_0019 /y1985/m10/d20 table 729 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0098 HAL_0019 /y1985/m10/d20 table 730 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0098 HAL_0019 /y1985/m10/d20 table 731 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0098 HAL_0019 /y1985/m10/d20 table 732 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0098 HAL_0019 /y1985/m10/d20 table 733 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0098 HAL_0019 /y1985/m10/d20 table 734 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0098 HAL_0019 /y1985/m10/d20 table 735 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0098 HAL_0019 /y1985/m10/d20 table 736 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0099 HAL_0019 /y1985/m10/d20 table 737 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0099 HAL_0019 /y1985/m10/d20 table 738 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0099 HAL_0019 /y1985/m10/d20 table 739 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0099 HAL_0019 /y1985/m10/d20 table 740 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0099 HAL_0019 /y1985/m10/d20 table 741 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0099 HAL_0019 /y1985/m10/d20 table 742 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0099 HAL_0019 /y1985/m10/d20 table 743 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0099 HAL_0019 /y1985/m10/d20 table 744 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0100 HAL_0019 /y1985/m10/d20 table 745 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0100 HAL_0019 /y1985/m10/d20 table 746 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0100 HAL_0019 /y1985/m10/d20 table 747 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0100 HAL_0019 /y1985/m10/d20 table 748 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0100 HAL_0019 /y1985/m10/d20 table 749 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0100 HAL_0019 /y1985/m10/d20 table 750 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0100 HAL_0019 /y1985/m10/d20 table 751 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0100 HAL_0019 /y1985/m10/d20 table 752 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0101 HAL_0019 /y1985/m10/d20 table 753 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0101 HAL_0019 /y1985/m10/d20 table 754 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0101 HAL_0019 /y1985/m10/d20 table 755 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0101 HAL_0019 /y1985/m10/d20 table 756 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0101 HAL_0019 /y1985/m10/d20 table 757 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0101 HAL_0019 /y1985/m10/d20 table 758 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0101 HAL_0019 /y1985/m10/d20 table 759 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0101 HAL_0019 /y1985/m10/d20 table 760 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0102 HAL_0019 /y1985/m10/d20 table 761 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0102 HAL_0019 /y1985/m10/d20 table 762 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0102 HAL_0019 /y1985/m10/d20 table 763 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0102 HAL_0019 /y1985/m10/d20 table 764 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0102 HAL_0019 /y1985/m10/d20 table 765 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0102 HAL_0019 /y1985/m10/d20 table 766 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0102 HAL_0019 /y1985/m10/d20 table 767 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0102 HAL_0019 /y1985/m10/d20 table 768 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0103 HAL_0019 /y1985/m10/d20 table 769 Used their k's (from raw data sheet), added
INTERP1** dM's as X=0 Mi-Ms star entries, then
calculated dM's and error (dM) from mean and
sdev
pflx0110 HAL_0019 /y1985/m11/d01 table 806 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0110 HAL_0019 /y1985/m11/d01 table 807 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0110 HAL_0019 /y1985/m11/d01 table 808 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0110 HAL_0019 /y1985/m11/d01 table 809 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0110 HAL_0019 /y1985/m11/d01 table 810 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0110 HAL_0019 /y1985/m11/d01 table 811 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0110 HAL_0019 /y1985/m11/d01 table 812 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0110 HAL_0019 /y1985/m11/d01 table 813 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0111 HAL_0019 /y1985/m11/d01 table 814 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0111 HAL_0019 /y1985/m11/d01 table 815 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0111 HAL_0019 /y1985/m11/d01 table 816 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0111 HAL_0019 /y1985/m11/d01 table 817 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0111 HAL_0019 /y1985/m11/d01 table 818 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0111 HAL_0019 /y1985/m11/d01 table 819 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0111 HAL_0019 /y1985/m11/d01 table 820 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0111 HAL_0019 /y1985/m11/d01 table 821 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0112 HAL_0019 /y1985/m11/d01 table 822 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0112 HAL_0019 /y1985/m11/d01 table 823 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0112 HAL_0019 /y1985/m11/d01 table 824 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0112 HAL_0019 /y1985/m11/d01 table 825 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0112 HAL_0019 /y1985/m11/d01 table 826 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0112 HAL_0019 /y1985/m11/d01 table 827 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0112 HAL_0019 /y1985/m11/d01 table 828 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0112 HAL_0019 /y1985/m11/d01 table 829 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0113 HAL_0019 /y1985/m11/d01 table 830 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0113 HAL_0019 /y1985/m11/d01 table 831 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0113 HAL_0019 /y1985/m11/d01 table 832 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0113 HAL_0019 /y1985/m11/d01 table 833 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0113 HAL_0019 /y1985/m11/d01 table 834 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0113 HAL_0019 /y1985/m11/d01 table 835 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0113 HAL_0019 /y1985/m11/d01 table 836 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0113 HAL_0019 /y1985/m11/d01 table 837 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0114 HAL_0019 /y1985/m11/d01 table 838 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0114 HAL_0019 /y1985/m11/d01 table 839 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0114 HAL_0019 /y1985/m11/d01 table 840 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0114 HAL_0019 /y1985/m11/d01 table 841 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0114 HAL_0019 /y1985/m11/d01 table 842 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0114 HAL_0019 /y1985/m11/d01 table 843 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0114 HAL_0019 /y1985/m11/d01 table 844 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0114 HAL_0019 /y1985/m11/d01 table 845 Calculated k's separately for HD34078 (original
X's) and HD52266 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0115 HAL_0019 /y1985/m11/d03 table 846 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0115 HAL_0019 /y1985/m11/d03 table 847 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0115 HAL_0019 /y1985/m11/d03 table 848 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0115 HAL_0019 /y1985/m11/d03 table 849 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0115 HAL_0019 /y1985/m11/d03 table 850 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0115 HAL_0019 /y1985/m11/d03 table 851 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0115 HAL_0019 /y1985/m11/d03 table 852 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0115 HAL_0019 /y1985/m11/d03 table 853 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0116 HAL_0019 /y1985/m11/d03 table 854 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0116 HAL_0019 /y1985/m11/d03 table 855 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0116 HAL_0019 /y1985/m11/d03 table 856 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0116 HAL_0019 /y1985/m11/d03 table 857 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0116 HAL_0019 /y1985/m11/d03 table 858 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0116 HAL_0019 /y1985/m11/d03 table 859 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0116 HAL_0019 /y1985/m11/d03 table 860 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0116 HAL_0019 /y1985/m11/d03 table 861 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0117 HAL_0019 /y1985/m11/d03 table 862 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0117 HAL_0019 /y1985/m11/d03 table 863 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0117 HAL_0019 /y1985/m11/d03 table 864 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0117 HAL_0019 /y1985/m11/d03 table 865 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0117 HAL_0019 /y1985/m11/d03 table 866 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0117 HAL_0019 /y1985/m11/d03 table 867 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0117 HAL_0019 /y1985/m11/d03 table 868 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0117 HAL_0019 /y1985/m11/d03 table 869 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
pflx0130 HAL_0019 /y1985/m11/d05 table 945 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0130 HAL_0019 /y1985/m11/d05 table 946 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0130 HAL_0019 /y1985/m11/d05 table 947 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0130 HAL_0019 /y1985/m11/d05 table 948 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0130 HAL_0019 /y1985/m11/d05 table 949 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0130 HAL_0019 /y1985/m11/d05 table 950 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0130 HAL_0019 /y1985/m11/d05 table 951 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0130 HAL_0019 /y1985/m11/d05 table 952 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0131 HAL_0019 /y1985/m11/d05 table 953 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0131 HAL_0019 /y1985/m11/d05 table 954 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0131 HAL_0019 /y1985/m11/d05 table 955 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0131 HAL_0019 /y1985/m11/d05 table 956 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0131 HAL_0019 /y1985/m11/d05 table 957 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0131 HAL_0019 /y1985/m11/d05 table 958 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0131 HAL_0019 /y1985/m11/d05 table 959 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0131 HAL_0019 /y1985/m11/d05 table 960 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0132 HAL_0019 /y1985/m11/d05 table 961 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0132 HAL_0019 /y1985/m11/d05 table 962 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0132 HAL_0019 /y1985/m11/d05 table 963 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0132 HAL_0019 /y1985/m11/d05 table 964 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0132 HAL_0019 /y1985/m11/d05 table 965 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0132 HAL_0019 /y1985/m11/d05 table 966 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0132 HAL_0019 /y1985/m11/d05 table 967 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0132 HAL_0019 /y1985/m11/d05 table 968 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0133 HAL_0019 /y1985/m11/d05 table 969 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0133 HAL_0019 /y1985/m11/d05 table 970 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0133 HAL_0019 /y1985/m11/d05 table 971 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0133 HAL_0019 /y1985/m11/d05 table 972 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0133 HAL_0019 /y1985/m11/d05 table 973 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0133 HAL_0019 /y1985/m11/d05 table 974 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0133 HAL_0019 /y1985/m11/d05 table 975 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0133 HAL_0019 /y1985/m11/d05 table 976 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0134 HAL_0019 /y1985/m11/d05 table 977 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0134 HAL_0019 /y1985/m11/d05 table 978 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0134 HAL_0019 /y1985/m11/d05 table 979 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0134 HAL_0019 /y1985/m11/d05 table 980 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0134 HAL_0019 /y1985/m11/d05 table 981 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0134 HAL_0019 /y1985/m11/d05 table 982 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0134 HAL_0019 /y1985/m11/d05 table 983 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0134 HAL_0019 /y1985/m11/d05 table 984 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0135 HAL_0019 /y1985/m11/d05 table 985 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0135 HAL_0019 /y1985/m11/d05 table 986 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0135 HAL_0019 /y1985/m11/d05 table 987 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0135 HAL_0019 /y1985/m11/d05 table 988 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0135 HAL_0019 /y1985/m11/d05 table 989 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0135 HAL_0019 /y1985/m11/d05 table 990 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0135 HAL_0019 /y1985/m11/d05 table 991 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0135 HAL_0019 /y1985/m11/d05 table 992 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0136 HAL_0019 /y1985/m11/d05 table 993 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0136 HAL_0019 /y1985/m11/d05 table 994 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0136 HAL_0019 /y1985/m11/d05 table 995 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0136 HAL_0019 /y1985/m11/d05 table 996 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0136 HAL_0019 /y1985/m11/d05 table 997 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0136 HAL_0019 /y1985/m11/d05 table 998 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0136 HAL_0019 /y1985/m11/d05 table 999 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0136 HAL_0019 /y1985/m11/d05 table 1000 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0137 HAL_0019 /y1985/m11/d05 table 1001 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0137 HAL_0019 /y1985/m11/d05 table 1002 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0137 HAL_0019 /y1985/m11/d05 table 1003 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0137 HAL_0019 /y1985/m11/d05 table 1004 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0137 HAL_0019 /y1985/m11/d05 table 1005 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0137 HAL_0019 /y1985/m11/d05 table 1006 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0137 HAL_0019 /y1985/m11/d05 table 1007 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0137 HAL_0019 /y1985/m11/d05 table 1008 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0138 HAL_0019 /y1985/m11/d05 table 1009 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0138 HAL_0019 /y1985/m11/d05 table 1010 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0138 HAL_0019 /y1985/m11/d05 table 1011 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0138 HAL_0019 /y1985/m11/d05 table 1012 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0138 HAL_0019 /y1985/m11/d05 table 1013 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0138 HAL_0019 /y1985/m11/d05 table 1014 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0138 HAL_0019 /y1985/m11/d05 table 1015 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
pflx0138 HAL_0019 /y1985/m11/d05 table 1016 Calculated k's separately for HD25680 and
HD52266 using X's from PHOTOM*, used mean
and sdev to get k, error (k), used these k's to
calc dM for each star, mean and sdev to get dM
and error (dM)
PLFX0141 1033 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0141 1034 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0141 1035 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0141 1036 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0141 1037 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0141 1038 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0141 1039 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0141 1040 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0142 1041 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0142 1042 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0142 1043 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0142 1044 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0142 1045 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0142 1046 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0142 1047 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0142 1048 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0143 1049 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0143 1050 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0143 1051 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0143 1052 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0143 1053 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0143 1054 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0143 1055 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0143 1056 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0144 1057 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0144 1058 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0144 1059 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0144 1060 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0144 1061 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0144 1062 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0144 1063 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0144 1064 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0145 1065 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0145 1066 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0145 1067 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0145 1068 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0145 1069 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0145 1070 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0145 1071 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0145 1072 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0146 1073 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0146 1074 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0146 1075 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0146 1076 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0146 1077 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0146 1078 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0146 1079 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0146 1080 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0147 1081 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0147 1082 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0147 1083 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0147 1084 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0147 1085 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0147 1086 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0147 1087 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0147 1088 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0148 1089 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0148 1090 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0148 1091 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0148 1092 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0148 1093 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0148 1094 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0148 1095 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0148 1096 Calculated k's separately for HD34078 (original
X's) and HD25680 (PHOTOM* X's), mean and sdev
to get k, error (k), used these k's to calc dM
for each star, mean and sdev to get dM and
error (dM)
PLFX0189 1320 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0189 1322 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0189 1324 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0189 1326 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0189 1327 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0189 1329 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0189 1331 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0189 1332 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0190 1333 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0190 1334 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0190 1335 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0190 1336 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0190 1337 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0190 1338 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0190 1339 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
PLFX0190 1340 No stars available to calculate k's separately,
fits are nice so just used k's and dM's from
combined fit to HD34078 (original X's) and
HD3379 and HD219188 (PHOTOM* X's)
pflx0251 HAL_0019 /y1985/m11/d12/h12 table 1661 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0251 HAL_0019 /y1985/m11/d12/h12 table 1662 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0251 HAL_0019 /y1985/m11/d12/h12 table 1663 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0251 HAL_0019 /y1985/m11/d12/h12 table 1664 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0251 HAL_0019 /y1985/m11/d12/h12 table 1665 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0251 HAL_0019 /y1985/m11/d12/h12 table 1666 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0251 HAL_0019 /y1985/m11/d12/h12 table 1667 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0251 HAL_0019 /y1985/m11/d12/h12 table 1668 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0252 HAL_0019 /y1985/m11/d12/h12 table 1669 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0252 HAL_0019 /y1985/m11/d12/h12 table 1670 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0252 HAL_0019 /y1985/m11/d12/h12 table 1671 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0252 HAL_0019 /y1985/m11/d12/h12 table 1672 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0252 HAL_0019 /y1985/m11/d12/h12 table 1673 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0252 HAL_0019 /y1985/m11/d12/h12 table 1674 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0252 HAL_0019 /y1985/m11/d12/h12 table 1675 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0252 HAL_0019 /y1985/m11/d12/h12 table 1676 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0253 HAL_0019 /y1985/m11/d12/h12 table 1677 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0253 HAL_0019 /y1985/m11/d12/h12 table 1678 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0253 HAL_0019 /y1985/m11/d12/h12 table 1679 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0253 HAL_0019 /y1985/m11/d12/h12 table 1680 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0253 HAL_0019 /y1985/m11/d12/h12 table 1681 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0253 HAL_0019 /y1985/m11/d12/h12 table 1682 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0253 HAL_0019 /y1985/m11/d12/h12 table 1683 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0253 HAL_0019 /y1985/m11/d12/h12 table 1684 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0254 HAL_0019 /y1985/m11/d12/h12 table 1685 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0254 HAL_0019 /y1985/m11/d12/h12 table 1686 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0254 HAL_0019 /y1985/m11/d12/h12 table 1687 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0254 HAL_0019 /y1985/m11/d12/h12 table 1688 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0254 HAL_0019 /y1985/m11/d12/h12 table 1689 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0254 HAL_0019 /y1985/m11/d12/h12 table 1690 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0254 HAL_0019 /y1985/m11/d12/h12 table 1691 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0254 HAL_0019 /y1985/m11/d12/h12 table 1692 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0255 HAL_0019 /y1985/m11/d12/h12 table 1693 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0255 HAL_0019 /y1985/m11/d12/h12 table 1694 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0255 HAL_0019 /y1985/m11/d12/h12 table 1695 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0255 HAL_0019 /y1985/m11/d12/h12 table 1696 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0255 HAL_0019 /y1985/m11/d12/h12 table 1697 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0255 HAL_0019 /y1985/m11/d12/h12 table 1698 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0255 HAL_0019 /y1985/m11/d12/h12 table 1699 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0255 HAL_0019 /y1985/m11/d12/h12 table 1700 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0256 HAL_0019 /y1985/m11/d12/h12 table 1701 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0256 HAL_0019 /y1985/m11/d12/h12 table 1702 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0256 HAL_0019 /y1985/m11/d12/h12 table 1703 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0256 HAL_0019 /y1985/m11/d12/h12 table 1704 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0256 HAL_0019 /y1985/m11/d12/h12 table 1705 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0256 HAL_0019 /y1985/m11/d12/h12 table 1706 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0256 HAL_0019 /y1985/m11/d12/h12 table 1707 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0256 HAL_0019 /y1985/m11/d12/h12 table 1708 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0257 HAL_0019 /y1985/m11/d12/h12 table 1709 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0257 HAL_0019 /y1985/m11/d12/h12 table 1710 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0257 HAL_0019 /y1985/m11/d12/h12 table 1711 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0257 HAL_0019 /y1985/m11/d12/h12 table 1712 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0257 HAL_0019 /y1985/m11/d12/h12 table 1713 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0257 HAL_0019 /y1985/m11/d12/h12 table 1714 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0257 HAL_0019 /y1985/m11/d12/h12 table 1715 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0257 HAL_0019 /y1985/m11/d12/h12 table 1716 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0258 HAL_0019 /y1985/m11/d12/h12 table 1717 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0258 HAL_0019 /y1985/m11/d12/h12 table 1718 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0258 HAL_0019 /y1985/m11/d12/h12 table 1719 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0258 HAL_0019 /y1985/m11/d12/h12 table 1720 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0258 HAL_0019 /y1985/m11/d12/h12 table 1721 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0258 HAL_0019 /y1985/m11/d12/h12 table 1722 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0258 HAL_0019 /y1985/m11/d12/h12 table 1723 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0258 HAL_0019 /y1985/m11/d12/h12 table 1724 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error (k), used these k's to calc dM for each star,
mean and sdev to get dM and error (dM)
pflx0259 HAL_0019 /y1985/m11/d13/h00 table 1725 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0259 HAL_0019 /y1985/m11/d13/h00 table 1726 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0259 HAL_0019 /y1985/m11/d13/h00 table 1727 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0259 HAL_0019 /y1985/m11/d13/h00 table 1728 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0259 HAL_0019 /y1985/m11/d13/h00 table 1729 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0259 HAL_0019 /y1985/m11/d13/h00 table 1730 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0259 HAL_0019 /y1985/m11/d13/h00 table 1731 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0259 HAL_0019 /y1985/m11/d13/h00 table 1732 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0260 HAL_0019 /y1985/m11/d13/h12 table 1733 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0260 HAL_0019 /y1985/m11/d13/h12 table 1734 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0260 HAL_0019 /y1985/m11/d13/h12 table 1735 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0260 HAL_0019 /y1985/m11/d13/h12 table 1736 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0260 HAL_0019 /y1985/m11/d13/h12 table 1737 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0260 HAL_0019 /y1985/m11/d13/h12 table 1738 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0260 HAL_0019 /y1985/m11/d13/h12 table 1739 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0260 HAL_0019 /y1985/m11/d13/h12 table 1740 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0261 HAL_0019 /y1985/m11/d13/h12 table 1741 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0261 HAL_0019 /y1985/m11/d13/h12 table 1742 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0261 HAL_0019 /y1985/m11/d13/h12 table 1743 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0261 HAL_0019 /y1985/m11/d13/h12 table 1744 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0261 HAL_0019 /y1985/m11/d13/h12 table 1745 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0261 HAL_0019 /y1985/m11/d13/h12 table 1746 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0261 HAL_0019 /y1985/m11/d13/h12 table 1747 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0261 HAL_0019 /y1985/m11/d13/h12 table 1748 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0262 HAL_0019 /y1985/m11/d13/h12 table 1749 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0262 HAL_0019 /y1985/m11/d13/h12 table 1750 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0262 HAL_0019 /y1985/m11/d13/h12 table 1751 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0262 HAL_0019 /y1985/m11/d13/h12 table 1752 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0262 HAL_0019 /y1985/m11/d13/h12 table 1753 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0262 HAL_0019 /y1985/m11/d13/h12 table 1754 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0262 HAL_0019 /y1985/m11/d13/h12 table 1755 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0262 HAL_0019 /y1985/m11/d13/h12 table 1756 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0263 HAL_0019 /y1985/m11/d13/h12 table 1757 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0263 HAL_0019 /y1985/m11/d13/h12 table 1758 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0263 HAL_0019 /y1985/m11/d13/h12 table 1759 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0263 HAL_0019 /y1985/m11/d13/h12 table 1760 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0263 HAL_0019 /y1985/m11/d13/h12 table 1761 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0263 HAL_0019 /y1985/m11/d13/h12 table 1762 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0263 HAL_0019 /y1985/m11/d13/h12 table 1763 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0263 HAL_0019 /y1985/m11/d13/h12 table 1764 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0264 HAL_0019 /y1985/m11/d13/h12 table 1765 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0264 HAL_0019 /y1985/m11/d13/h12 table 1766 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0264 HAL_0019 /y1985/m11/d13/h12 table 1767 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0264 HAL_0019 /y1985/m11/d13/h12 table 1768 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0264 HAL_0019 /y1985/m11/d13/h12 table 1769 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0264 HAL_0019 /y1985/m11/d13/h12 table 1770 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0264 HAL_0019 /y1985/m11/d13/h12 table 1771 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0264 HAL_0019 /y1985/m11/d13/h12 table 1772 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0265 HAL_0019 /y1985/m11/d13/h12 table 1773 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0265 HAL_0019 /y1985/m11/d13/h12 table 1774 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0265 HAL_0019 /y1985/m11/d13/h12 table 1775 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0265 HAL_0019 /y1985/m11/d13/h12 table 1776 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0265 HAL_0019 /y1985/m11/d13/h12 table 1777 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0265 HAL_0019 /y1985/m11/d13/h12 table 1778 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0265 HAL_0019 /y1985/m11/d13/h12 table 1779 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0265 HAL_0019 /y1985/m11/d13/h12 table 1780 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0266 HAL_0019 /y1985/m11/d13/h12 table 1781 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0266 HAL_0019 /y1985/m11/d13/h12 table 1782 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0266 HAL_0019 /y1985/m11/d13/h12 table 1783 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0266 HAL_0019 /y1985/m11/d13/h12 table 1784 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0266 HAL_0019 /y1985/m11/d13/h12 table 1785 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0266 HAL_0019 /y1985/m11/d13/h12 table 1786 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0266 HAL_0019 /y1985/m11/d13/h12 table 1787 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0266 HAL_0019 /y1985/m11/d13/h12 table 1788 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0267 HAL_0019 /y1985/m11/d13/h12 table 1789 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0267 HAL_0019 /y1985/m11/d13/h12 table 1790 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0267 HAL_0019 /y1985/m11/d13/h12 table 1791 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0267 HAL_0019 /y1985/m11/d13/h12 table 1792 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0267 HAL_0019 /y1985/m11/d13/h12 table 1793 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0267 HAL_0019 /y1985/m11/d13/h12 table 1794 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0267 HAL_0019 /y1985/m11/d13/h12 table 1795 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0267 HAL_0019 /y1985/m11/d13/h12 table 1796 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0268 HAL_0019 /y1985/m11/d13/h12 table 1797 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0268 HAL_0019 /y1985/m11/d13/h12 table 1798 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0268 HAL_0019 /y1985/m11/d13/h12 table 1799 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0268 HAL_0019 /y1985/m11/d13/h12 table 1800 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0268 HAL_0019 /y1985/m11/d13/h12 table 1801 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0268 HAL_0019 /y1985/m11/d13/h12 table 1802 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0268 HAL_0019 /y1985/m11/d13/h12 table 1803 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0268 HAL_0019 /y1985/m11/d13/h12 table 1804 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0269 HAL_0019 /y1985/m11/d13/h12 table 1805 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0269 HAL_0019 /y1985/m11/d13/h12 table 1806 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0269 HAL_0019 /y1985/m11/d13/h12 table 1807 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0269 HAL_0019 /y1985/m11/d13/h12 table 1808 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0269 HAL_0019 /y1985/m11/d13/h12 table 1809 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0269 HAL_0019 /y1985/m11/d13/h12 table 1810 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0269 HAL_0019 /y1985/m11/d13/h12 table 1811 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0269 HAL_0019 /y1985/m11/d13/h12 table 1812 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0270 HAL_0019 /y1985/m11/d13/h12 table 1813 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0270 HAL_0019 /y1985/m11/d13/h12 table 1814 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0270 HAL_0019 /y1985/m11/d13/h12 table 1815 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0270 HAL_0019 /y1985/m11/d13/h12 table 1816 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0270 HAL_0019 /y1985/m11/d13/h12 table 1817 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0270 HAL_0019 /y1985/m11/d13/h12 table 1818 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0270 HAL_0019 /y1985/m11/d13/h12 table 1819 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0270 HAL_0019 /y1985/m11/d13/h12 table 1820 Fits are nice so just used k's and dM's from combined
fit to HD3379 and HD25680 using PHOTOM* X's
pflx0272 HAL_0019 /y1985/m11/d14/h12 table 1826 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0272 HAL_0019 /y1985/m11/d14/h12 table 1827 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0272 HAL_0019 /y1985/m11/d14/h12 table 1828 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0272 HAL_0019 /y1985/m11/d14/h12 table 1829 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0272 HAL_0019 /y1985/m11/d14/h12 table 1830 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0272 HAL_0019 /y1985/m11/d14/h12 table 1831 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0272 HAL_0019 /y1985/m11/d14/h12 table 1832 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0272 HAL_0019 /y1985/m11/d14/h12 table 1833 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0273 HAL_0019 /y1985/m11/d14/h12 table 1834 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0273 HAL_0019 /y1985/m11/d14/h12 table 1835 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0273 HAL_0019 /y1985/m11/d14/h12 table 1836 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0273 HAL_0019 /y1985/m11/d14/h12 table 1837 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0273 HAL_0019 /y1985/m11/d14/h12 table 1838 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0273 HAL_0019 /y1985/m11/d14/h12 table 1839 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0273 HAL_0019 /y1985/m11/d14/h12 table 1840 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0273 HAL_0019 /y1985/m11/d14/h12 table 1841 No way to calculate k from individual star, so
averaged dM's from 51113 (11/13/85) and 51115
(11/15/85) to get dM, error(dM), then predicted
k's from those dM's, k's are simialer to those
found on 51113 and 51115, used 0.01 for error(k)
pflx0283 HAL_0019 /y1985/m11/d15/h12 table 1901 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0283 HAL_0019 /y1985/m11/d15/h12 table 1903 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0283 HAL_0019 /y1985/m11/d15/h12 table 1904 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0283 HAL_0019 /y1985/m11/d15/h12 table 1906 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0283 HAL_0019 /y1985/m11/d15/h12 table 1907 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0283 HAL_0019 /y1985/m11/d15/h12 table 1908 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0283 HAL_0019 /y1985/m11/d15/h12 table 1910 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0283 HAL_0019 /y1985/m11/d15/h12 table 1911 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0285 HAL_0019 /y1985/m11/d15/h12 table 1916 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0285 HAL_0019 /y1985/m11/d15/h12 table 1917 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0285 HAL_0019 /y1985/m11/d15/h12 table 1918 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0285 HAL_0019 /y1985/m11/d15/h12 table 1919 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0285 HAL_0019 /y1985/m11/d15/h12 table 1920 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0285 HAL_0019 /y1985/m11/d15/h12 table 1921 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0285 HAL_0019 /y1985/m11/d15/h12 table 1922 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0285 HAL_0019 /y1985/m11/d15/h12 table 1923 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0286 HAL_0019 /y1985/m11/d15/h12 table 1924 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0286 HAL_0019 /y1985/m11/d15/h12 table 1925 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0286 HAL_0019 /y1985/m11/d15/h12 table 1926 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0286 HAL_0019 /y1985/m11/d15/h12 table 1927 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0286 HAL_0019 /y1985/m11/d15/h12 table 1928 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0286 HAL_0019 /y1985/m11/d15/h12 table 1929 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0286 HAL_0019 /y1985/m11/d15/h12 table 1930 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0286 HAL_0019 /y1985/m11/d15/h12 table 1931 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0287 HAL_0019 /y1985/m11/d15/h12 table 1932 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0287 HAL_0019 /y1985/m11/d15/h12 table 1933 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0287 HAL_0019 /y1985/m11/d15/h12 table 1934 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0287 HAL_0019 /y1985/m11/d15/h12 table 1936 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0287 HAL_0019 /y1985/m11/d15/h12 table 1937 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0287 HAL_0019 /y1985/m11/d15/h12 table 1939 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0287 HAL_0019 /y1985/m11/d15/h12 table 1941 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0287 HAL_0019 /y1985/m11/d15/h12 table 1942 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0289 HAL_0019 /y1985/m11/d15/h12 table 1946 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0289 HAL_0019 /y1985/m11/d15/h12 table 1947 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0289 HAL_0019 /y1985/m11/d15/h12 table 1948 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0289 HAL_0019 /y1985/m11/d15/h12 table 1949 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0289 HAL_0019 /y1985/m11/d15/h12 table 1950 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0289 HAL_0019 /y1985/m11/d15/h12 table 1951 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0289 HAL_0019 /y1985/m11/d15/h12 table 1952 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0289 HAL_0019 /y1985/m11/d15/h12 table 1953 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0290 HAL_0019 /y1985/m11/d15/h12 table 1954 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0290 HAL_0019 /y1985/m11/d15/h12 table 1955 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0290 HAL_0019 /y1985/m11/d15/h12 table 1956 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0290 HAL_0019 /y1985/m11/d15/h12 table 1957 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0290 HAL_0019 /y1985/m11/d15/h12 table 1958 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0290 HAL_0019 /y1985/m11/d15/h12 table 1959 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0290 HAL_0019 /y1985/m11/d15/h12 table 1960 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0290 HAL_0019 /y1985/m11/d15/h12 table 1961 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0291 HAL_0019 /y1985/m11/d15/h12 table 1962 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0291 HAL_0019 /y1985/m11/d15/h12 table 1963 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0291 HAL_0019 /y1985/m11/d15/h12 table 1964 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0291 HAL_0019 /y1985/m11/d15/h12 table 1965 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0291 HAL_0019 /y1985/m11/d15/h12 table 1966 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0291 HAL_0019 /y1985/m11/d15/h12 table 1967 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0291 HAL_0019 /y1985/m11/d15/h12 table 1968 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0291 HAL_0019 /y1985/m11/d15/h12 table 1969 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0292 HAL_0019 /y1985/m11/d15/h12 table 1970 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0292 HAL_0019 /y1985/m11/d15/h12 table 1971 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0292 HAL_0019 /y1985/m11/d15/h12 table 1972 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0292 HAL_0019 /y1985/m11/d15/h12 table 1973 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0292 HAL_0019 /y1985/m11/d15/h12 table 1974 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0292 HAL_0019 /y1985/m11/d15/h12 table 1975 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0292 HAL_0019 /y1985/m11/d15/h12 table 1976 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0292 HAL_0019 /y1985/m11/d15/h12 table 1977 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0293 HAL_0019 /y1985/m11/d15/h12 table 1978 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0293 HAL_0019 /y1985/m11/d15/h12 table 1979 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0293 HAL_0019 /y1985/m11/d15/h12 table 1980 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0293 HAL_0019 /y1985/m11/d15/h12 table 1981 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0293 HAL_0019 /y1985/m11/d15/h12 table 1982 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0293 HAL_0019 /y1985/m11/d15/h12 table 1983 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0293 HAL_0019 /y1985/m11/d15/h12 table 1984 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0293 HAL_0019 /y1985/m11/d15/h12 table 1985 Omitted HD52266 and fit all 4 entries for HD25680
together to get k's and dM's, not much airmass
covered, but k's are more reasonable than if HD52266
were included
pflx0328 HAL_0019 /y1985/m11/d17/h12 table 2173 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0328 HAL_0019 /y1985/m11/d17/h12 table 2174 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0328 HAL_0019 /y1985/m11/d17/h12 table 2175 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0328 HAL_0019 /y1985/m11/d17/h12 table 2176 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0328 HAL_0019 /y1985/m11/d17/h12 table 2177 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0328 HAL_0019 /y1985/m11/d17/h12 table 2179 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0328 HAL_0019 /y1985/m11/d17/h12 table 2181 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0328 HAL_0019 /y1985/m11/d17/h12 table 2184 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0330 HAL_0019 /y1985/m11/d17/h12 table 2187 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0330 HAL_0019 /y1985/m11/d17/h12 table 2188 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0330 HAL_0019 /y1985/m11/d17/h12 table 2189 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0330 HAL_0019 /y1985/m11/d17/h12 table 2190 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0330 HAL_0019 /y1985/m11/d17/h12 table 2191 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0330 HAL_0019 /y1985/m11/d17/h12 table 2192 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0330 HAL_0019 /y1985/m11/d17/h12 table 2193 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0330 HAL_0019 /y1985/m11/d17/h12 table 2194 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0332 HAL_0019 /y1985/m11/d17/h12 table 2197 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0332 HAL_0019 /y1985/m11/d17/h12 table 2199 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0332 HAL_0019 /y1985/m11/d17/h12 table 2201 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0332 HAL_0019 /y1985/m11/d17/h12 table 2203 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0332 HAL_0019 /y1985/m11/d17/h12 table 2204 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0332 HAL_0019 /y1985/m11/d17/h12 table 2206 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0332 HAL_0019 /y1985/m11/d17/h12 table 2207 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0332 HAL_0019 /y1985/m11/d17/h12 table 2208 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0333 HAL_0019 /y1985/m11/d17/h12 table 2209 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0333 HAL_0019 /y1985/m11/d17/h12 table 2210 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0333 HAL_0019 /y1985/m11/d17/h12 table 2211 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0333 HAL_0019 /y1985/m11/d17/h12 table 2212 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0333 HAL_0019 /y1985/m11/d17/h12 table 2213 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0333 HAL_0019 /y1985/m11/d17/h12 table 2214 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0333 HAL_0019 /y1985/m11/d17/h12 table 2215 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0333 HAL_0019 /y1985/m11/d17/h12 table 2216 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0335 HAL_0019 /y1985/m11/d17/h12 table 2223 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0335 HAL_0019 /y1985/m11/d17/h12 table 2224 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0335 HAL_0019 /y1985/m11/d17/h12 table 2225 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0335 HAL_0019 /y1985/m11/d17/h12 table 2226 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0335 HAL_0019 /y1985/m11/d17/h12 table 2227 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0335 HAL_0019 /y1985/m11/d17/h12 table 2228 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0335 HAL_0019 /y1985/m11/d17/h12 table 2229 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0335 HAL_0019 /y1985/m11/d17/h12 table 2230 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0336 HAL_0019 /y1985/m11/d17/h12 table 2231 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0336 HAL_0019 /y1985/m11/d17/h12 table 2232 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0336 HAL_0019 /y1985/m11/d17/h12 table 2233 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0336 HAL_0019 /y1985/m11/d17/h12 table 2234 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0336 HAL_0019 /y1985/m11/d17/h12 table 2235 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0336 HAL_0019 /y1985/m11/d17/h12 table 2236 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0336 HAL_0019 /y1985/m11/d17/h12 table 2237 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0336 HAL_0019 /y1985/m11/d17/h12 table 2238 Calculated k's separately for HD3379 and HD25680
using PHOTOM* X's, used mean and sdev to get k,
error(k), used these k's to calc dM for each star,
mean and sdev to get dM and error(dM)
pflx0349 HAL_0019 /y1985/m11/d20 table 2323 Used INTERP2*** dM's to predict k for each star
entry, then used mean and sdev to get k, error(k),
used INTERP2*** dM's and errors
pflx0349 HAL_0019 /y1985/m11/d20 table 2324 Used INTERP2*** dM's to predict k for each star
entry, then used mean and sdev to get k, error(k),
used INTERP2*** dM's and errors
pflx0349 HAL_0019 /y1985/m11/d20 table 2325 Used INTERP2*** dM's to predict k for each star
entry, then used mean and sdev to get k, error(k),
used INTERP2*** dM's and errors
pflx0349 HAL_0019 /y1985/m11/d20 table 2326 Used INTERP2*** dM's to predict k for each star
entry, then used mean and sdev to get k, error(k),
used INTERP2*** dM's and errors
pflx0349 HAL_0019 /y1985/m11/d20 table 2327 Used INTERP2*** dM's to predict k for each star
entry, then used mean and sdev to get k, error(k),
used INTERP2*** dM's and errors
pflx0349 HAL_0019 /y1985/m11/d20 table 2328 Used INTERP2*** dM's to predict k for each star
entry, then used mean and sdev to get k, error(k),
used INTERP2*** dM's and errors
pflx0349 HAL_0019 /y1985/m11/d20 table 2329 Used INTERP2*** dM's to predict k for each star
entry, then used mean and sdev to get k, error(k),
used INTERP2*** dM's and errors
pflx0349 HAL_0019 /y1985/m11/d20 table 2330 Used INTERP2*** dM's to predict k for each star
entry, then used mean and sdev to get k, error(k),
used INTERP2*** dM's and errors
pflx0350 HAL_0019 /y1985/m11/d21 table 2331 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0350 HAL_0019 /y1985/m11/d21 table 2332 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0350 HAL_0019 /y1985/m11/d21 table 2333 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0350 HAL_0019 /y1985/m11/d21 table 2334 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0350 HAL_0019 /y1985/m11/d21 table 2335 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0350 HAL_0019 /y1985/m11/d21 table 2336 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0350 HAL_0019 /y1985/m11/d21 table 2337 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0351 HAL_0019 /y1985/m11/d21 table 2338 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0351 HAL_0019 /y1985/m11/d21 table 2339 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0351 HAL_0019 /y1985/m11/d21 table 2340 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0351 HAL_0019 /y1985/m11/d21 table 2341 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0351 HAL_0019 /y1985/m11/d21 table 2342 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0351 HAL_0019 /y1985/m11/d21 table 2343 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0351 HAL_0019 /y1985/m11/d21 table 2344 Used INTERP2*** dM's to predict k for the one star
entry to get k, used INTERP2*** dM's and errors, used
0.01 for error(k)
pflx0363 HAL_0019 /y1985/m11/d22 table 2406 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0363 HAL_0019 /y1985/m11/d22 table 2407 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0363 HAL_0019 /y1985/m11/d22 table 2408 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0363 HAL_0019 /y1985/m11/d22 table 2409 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0363 HAL_0019 /y1985/m11/d22 table 2410 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0363 HAL_0019 /y1985/m11/d22 table 2411 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0363 HAL_0019 /y1985/m11/d22 table 2412 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0363 HAL_0019 /y1985/m11/d22 table 2413 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0364 HAL_0019 /y1985/m11/d22 table 2414 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0364 HAL_0019 /y1985/m11/d22 table 2415 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0364 HAL_0019 /y1985/m11/d22 table 2416 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0364 HAL_0019 /y1985/m11/d22 table 2417 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0364 HAL_0019 /y1985/m11/d22 table 2418 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0364 HAL_0019 /y1985/m11/d22 table 2419 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0364 HAL_0019 /y1985/m11/d22 table 2420 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0364 HAL_0019 /y1985/m11/d22 table 2421 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0365 HAL_0019 /y1985/m11/d22 table 2422 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0365 HAL_0019 /y1985/m11/d22 table 2423 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0365 HAL_0019 /y1985/m11/d22 table 2424 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0365 HAL_0019 /y1985/m11/d22 table 2425 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0365 HAL_0019 /y1985/m11/d22 table 2426 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0365 HAL_0019 /y1985/m11/d22 table 2427 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0365 HAL_0019 /y1985/m11/d22 table 2428 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0365 HAL_0019 /y1985/m11/d22 table 2429 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0366 HAL_0019 /y1985/m11/d22 table 2430 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0366 HAL_0019 /y1985/m11/d22 table 2431 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0366 HAL_0019 /y1985/m11/d22 table 2432 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0366 HAL_0019 /y1985/m11/d22 table 2433 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0366 HAL_0019 /y1985/m11/d22 table 2434 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0366 HAL_0019 /y1985/m11/d22 table 2435 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0366 HAL_0019 /y1985/m11/d22 table 2436 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0366 HAL_0019 /y1985/m11/d22 table 2437 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0367 HAL_0019 /y1985/m11/d22 table 2438 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0367 HAL_0019 /y1985/m11/d22 table 2439 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0367 HAL_0019 /y1985/m11/d22 table 2440 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0367 HAL_0019 /y1985/m11/d22 table 2441 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0367 HAL_0019 /y1985/m11/d22 table 2442 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0367 HAL_0019 /y1985/m11/d22 table 2443 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0367 HAL_0019 /y1985/m11/d22 table 2444 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0367 HAL_0019 /y1985/m11/d22 table 2445 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0368 HAL_0019 /y1985/m11/d22 table 2446 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0368 HAL_0019 /y1985/m11/d22 table 2447 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0368 HAL_0019 /y1985/m11/d22 table 2448 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0368 HAL_0019 /y1985/m11/d22 table 2449 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0368 HAL_0019 /y1985/m11/d22 table 2450 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0368 HAL_0019 /y1985/m11/d22 table 2451 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0368 HAL_0019 /y1985/m11/d22 table 2452 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0368 HAL_0019 /y1985/m11/d22 table 2453 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD25680 using PHOTOM*
X's
pflx0415 HAL_0019 /y1985/m11/d29 table 2701 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0415 HAL_0019 /y1985/m11/d29 table 2702 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0415 HAL_0019 /y1985/m11/d29 table 2703 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0415 HAL_0019 /y1985/m11/d29 table 2704 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0415 HAL_0019 /y1985/m11/d29 table 2705 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0415 HAL_0019 /y1985/m11/d29 table 2706 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0415 HAL_0019 /y1985/m11/d29 table 2707 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0415 HAL_0019 /y1985/m11/d29 table 2708 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0416 HAL_0019 /y1985/m11/d29 table 2709 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0416 HAL_0019 /y1985/m11/d29 table 2710 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0416 HAL_0019 /y1985/m11/d29 table 2711 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0416 HAL_0019 /y1985/m11/d29 table 2712 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0416 HAL_0019 /y1985/m11/d29 table 2713 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0416 HAL_0019 /y1985/m11/d29 table 2714 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0416 HAL_0019 /y1985/m11/d29 table 2715 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0416 HAL_0019 /y1985/m11/d29 table 2716 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0417 HAL_0019 /y1985/m11/d29 table 2717 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0417 HAL_0019 /y1985/m11/d29 table 2718 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0417 HAL_0019 /y1985/m11/d29 table 2719 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0417 HAL_0019 /y1985/m11/d29 table 2720 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0417 HAL_0019 /y1985/m11/d29 table 2721 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0417 HAL_0019 /y1985/m11/d29 table 2722 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0417 HAL_0019 /y1985/m11/d29 table 2723 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0417 HAL_0019 /y1985/m11/d29 table 2724 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0418 HAL_0019 /y1985/m11/d29 table 2725 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0418 HAL_0019 /y1985/m11/d29 table 2726 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0418 HAL_0019 /y1985/m11/d29 table 2727 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0418 HAL_0019 /y1985/m11/d29 table 2728 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0418 HAL_0019 /y1985/m11/d29 table 2729 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0418 HAL_0019 /y1985/m11/d29 table 2730 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0418 HAL_0019 /y1985/m11/d29 table 2731 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0418 HAL_0019 /y1985/m11/d29 table 2732 Calculated k's separately for HD34078 (original
X's), HD3379 and HD25680 (PHOTOM* X's), used
mean and sdev to get k, error(k), used these k's
to calc dM for each star, mean and sdev to get
dM and error(dM)
pflx0428 HAL_0019 /y1985/m12/d01/h12 table 2778 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0428 HAL_0019 /y1985/m12/d01/h12 table 2779 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0428 HAL_0019 /y1985/m12/d01/h12 table 2780 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0428 HAL_0019 /y1985/m12/d01/h12 table 2781 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0428 HAL_0019 /y1985/m12/d01/h12 table 2782 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0428 HAL_0019 /y1985/m12/d01/h12 table 2783 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0428 HAL_0019 /y1985/m12/d01/h12 table 2784 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0428 HAL_0019 /y1985/m12/d01/h12 table 2785 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0429 HAL_0019 /y1985/m12/d01/h12 table 2786 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0429 HAL_0019 /y1985/m12/d01/h12 table 2787 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0429 HAL_0019 /y1985/m12/d01/h12 table 2788 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0429 HAL_0019 /y1985/m12/d01/h12 table 2789 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0429 HAL_0019 /y1985/m12/d01/h12 table 2790 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0429 HAL_0019 /y1985/m12/d01/h12 table 2791 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0429 HAL_0019 /y1985/m12/d01/h12 table 2792 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0429 HAL_0019 /y1985/m12/d01/h12 table 2793 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0430 HAL_0019 /y1985/m12/d01/h12 table 2794 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0430 HAL_0019 /y1985/m12/d01/h12 table 2795 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0430 HAL_0019 /y1985/m12/d01/h12 table 2796 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0430 HAL_0019 /y1985/m12/d01/h12 table 2797 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0430 HAL_0019 /y1985/m12/d01/h12 table 2798 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0430 HAL_0019 /y1985/m12/d01/h12 table 2799 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0430 HAL_0019 /y1985/m12/d01/h12 table 2800 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0430 HAL_0019 /y1985/m12/d01/h12 table 2801 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0431 HAL_0019 /y1985/m12/d01/h12 table 2802 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0431 HAL_0019 /y1985/m12/d01/h12 table 2803 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0431 HAL_0019 /y1985/m12/d01/h12 table 2804 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0431 HAL_0019 /y1985/m12/d01/h12 table 2805 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0431 HAL_0019 /y1985/m12/d01/h12 table 2806 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0431 HAL_0019 /y1985/m12/d01/h12 table 2807 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0431 HAL_0019 /y1985/m12/d01/h12 table 2808 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0431 HAL_0019 /y1985/m12/d01/h12 table 2809 Used HD3379 to calculate k, dM together, values
look okay, used 0.01 for error(k) and error(dM)
pflx0490 HAL_0020 /y1985/m12/d09/h15 table 3169 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0490 HAL_0020 /y1985/m12/d09/h15 table 3170 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0490 HAL_0020 /y1985/m12/d09/h15 table 3171 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0490 HAL_0020 /y1985/m12/d09/h15 table 3172 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0490 HAL_0020 /y1985/m12/d09/h15 table 3173 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0490 HAL_0020 /y1985/m12/d09/h15 table 3174 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0490 HAL_0020 /y1985/m12/d09/h15 table 3175 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0490 HAL_0020 /y1985/m12/d09/h15 table 3176 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0491 HAL_0020 /y1985/m12/d09/h15 table 3177 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0491 HAL_0020 /y1985/m12/d09/h15 table 3178 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0491 HAL_0020 /y1985/m12/d09/h15 table 3179 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0491 HAL_0020 /y1985/m12/d09/h15 table 3180 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0491 HAL_0020 /y1985/m12/d09/h15 table 3181 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0491 HAL_0020 /y1985/m12/d09/h15 table 3182 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0491 HAL_0020 /y1985/m12/d09/h15 table 3183 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0491 HAL_0020 /y1985/m12/d09/h15 table 3184 Used HD25680 to calculate k's, estimated
error(k)=0.01, used these k's to predict dM for
each star entry, mean and sdev to get dM and
error(dM)
pflx0500 HAL_0020 /y1985/m12/d10/h12 table 3228 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0500 HAL_0020 /y1985/m12/d10/h12 table 3229 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0500 HAL_0020 /y1985/m12/d10/h12 table 3230 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0500 HAL_0020 /y1985/m12/d10/h12 table 3231 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0500 HAL_0020 /y1985/m12/d10/h12 table 3232 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0500 HAL_0020 /y1985/m12/d10/h12 table 3233 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0500 HAL_0020 /y1985/m12/d10/h12 table 3234 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0500 HAL_0020 /y1985/m12/d10/h12 table 3235 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM). Also, Sanglok data for this night,
12/10/85, 7000A Filter, Set 1 had the wrong
fraction of the day time in the input file,
and was changed from 0.7861 to 0.7028
pflx0501 HAL_0020 /y1985/m12/d10/h12 table 3236 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0501 HAL_0020 /y1985/m12/d10/h12 table 3237 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0501 HAL_0020 /y1985/m12/d10/h12 table 3238 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0501 HAL_0020 /y1985/m12/d10/h12 table 3239 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0501 HAL_0020 /y1985/m12/d10/h12 table 3240 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0501 HAL_0020 /y1985/m12/d10/h12 table 3241 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0501 HAL_0020 /y1985/m12/d10/h12 table 3242 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0501 HAL_0020 /y1985/m12/d10/h12 table 3243 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0502 HAL_0020 /y1985/m12/d10/h12 table 3244 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0502 HAL_0020 /y1985/m12/d10/h12 table 3245 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0502 HAL_0020 /y1985/m12/d10/h12 table 3246 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0502 HAL_0020 /y1985/m12/d10/h12 table 3247 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0502 HAL_0020 /y1985/m12/d10/h12 table 3248 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0502 HAL_0020 /y1985/m12/d10/h12 table 3249 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0502 HAL_0020 /y1985/m12/d10/h12 table 3250 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0502 HAL_0020 /y1985/m12/d10/h12 table 3251 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0503 HAL_0020 /y1985/m12/d10/h12 table 3252 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0503 HAL_0020 /y1985/m12/d10/h12 table 3253 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0503 HAL_0020 /y1985/m12/d10/h12 table 3254 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0503 HAL_0020 /y1985/m12/d10/h12 table 3255 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0503 HAL_0020 /y1985/m12/d10/h12 table 3256 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0503 HAL_0020 /y1985/m12/d10/h12 table 3257 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0503 HAL_0020 /y1985/m12/d10/h12 table 3258 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0503 HAL_0020 /y1985/m12/d10/h12 table 3259 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0504 HAL_0020 /y1985/m12/d11/h12 table 3260 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0504 HAL_0020 /y1985/m12/d11/h12 table 3261 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0504 HAL_0020 /y1985/m12/d11/h12 table 3262 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0504 HAL_0020 /y1985/m12/d11/h12 table 3263 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0504 HAL_0020 /y1985/m12/d11/h12 table 3264 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0504 HAL_0020 /y1985/m12/d11/h12 table 3265 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0504 HAL_0020 /y1985/m12/d11/h12 table 3266 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0504 HAL_0020 /y1985/m12/d11/h12 table 3267 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0505 HAL_0020 /y1985/m12/d11/h12 table 3268 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0505 HAL_0020 /y1985/m12/d11/h12 table 3269 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0505 HAL_0020 /y1985/m12/d11/h12 table 3270 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0505 HAL_0020 /y1985/m12/d11/h12 table 3271 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0505 HAL_0020 /y1985/m12/d11/h12 table 3272 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0505 HAL_0020 /y1985/m12/d11/h12 table 3273 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0505 HAL_0020 /y1985/m12/d11/h12 table 3274 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0505 HAL_0020 /y1985/m12/d11/h12 table 3275 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0533 HAL_0020 /y1985/m12/d15/h15 table 3436 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0533 HAL_0020 /y1985/m12/d15/h15 table 3437 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0533 HAL_0020 /y1985/m12/d15/h15 table 3438 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0533 HAL_0020 /y1985/m12/d15/h15 table 3439 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0533 HAL_0020 /y1985/m12/d15/h15 table 3440 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0533 HAL_0020 /y1985/m12/d15/h15 table 3441 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0533 HAL_0020 /y1985/m12/d15/h15 table 3442 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0533 HAL_0020 /y1985/m12/d15/h15 table 3443 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0534 HAL_0020 /y1985/m12/d15/h15 table 3444 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0534 HAL_0020 /y1985/m12/d15/h15 table 3445 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0534 HAL_0020 /y1985/m12/d15/h15 table 3446 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0534 HAL_0020 /y1985/m12/d15/h15 table 3447 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0534 HAL_0020 /y1985/m12/d15/h15 table 3448 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0534 HAL_0020 /y1985/m12/d15/h15 table 3449 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0534 HAL_0020 /y1985/m12/d15/h15 table 3450 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0534 HAL_0020 /y1985/m12/d15/h15 table 3451 Used HD34078 (original X's) and HD25680 to calc
k separately, then mean and sdev to get k,
error(k), used these k's to predict dM for each
star entry, then mean and sdev to get dM and
error(dM)
pflx0546 HAL_0020 /y1985/m12/d16/h12 table 3509 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0546 HAL_0020 /y1985/m12/d16/h12 table 3510 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0546 HAL_0020 /y1985/m12/d16/h12 table 3511 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0546 HAL_0020 /y1985/m12/d16/h12 table 3512 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0546 HAL_0020 /y1985/m12/d16/h12 table 3513 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0546 HAL_0020 /y1985/m12/d16/h12 table 3514 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0546 HAL_0020 /y1985/m12/d16/h12 table 3515 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0546 HAL_0020 /y1985/m12/d16/h12 table 3516 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0547 HAL_0020 /y1985/m12/d16/h12 table 3517 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0547 HAL_0020 /y1985/m12/d16/h12 table 3518 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0547 HAL_0020 /y1985/m12/d16/h12 table 3519 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0548 HAL_0020 /y1985/m12/d16/h12 table 3520 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0548 HAL_0020 /y1985/m12/d16/h12 table 3521 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0548 HAL_0020 /y1985/m12/d16/h12 table 3522 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0548 HAL_0020 /y1985/m12/d16/h12 table 3523 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0548 HAL_0020 /y1985/m12/d16/h12 table 3524 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0548 HAL_0020 /y1985/m12/d16/h12 table 3525 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0548 HAL_0020 /y1985/m12/d16/h12 table 3526 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0548 HAL_0020 /y1985/m12/d16/h12 table 3527 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0549 HAL_0020 /y1985/m12/d16/h12 table 3528 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0549 HAL_0020 /y1985/m12/d16/h12 table 3529 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0549 HAL_0020 /y1985/m12/d16/h12 table 3530 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0549 HAL_0020 /y1985/m12/d16/h12 table 3531 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0549 HAL_0020 /y1985/m12/d16/h12 table 3532 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0549 HAL_0020 /y1985/m12/d16/h12 table 3533 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0549 HAL_0020 /y1985/m12/d16/h12 table 3534 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0549 HAL_0020 /y1985/m12/d16/h12 table 3535 Used dM and error(dM) from 12/11/85, 51211,
estimated k and error(k) using these dM's and
data for HD3379
pflx0587 HAL_0020 /y1986/m01/d03 table 3752 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0587 HAL_0020 /y1986/m01/d03 table 3753 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0587 HAL_0020 /y1986/m01/d03 table 3754 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0587 HAL_0020 /y1986/m01/d03 table 3755 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0587 HAL_0020 /y1986/m01/d03 table 3756 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0587 HAL_0020 /y1986/m01/d03 table 3757 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0587 HAL_0020 /y1986/m01/d03 table 3758 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0587 HAL_0020 /y1986/m01/d03 table 3759 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0588 HAL_0020 /y1986/m01/d03 table 3760 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0588 HAL_0020 /y1986/m01/d03 table 3761 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0588 HAL_0020 /y1986/m01/d03 table 3762 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0588 HAL_0020 /y1986/m01/d03 table 3763 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0588 HAL_0020 /y1986/m01/d03 table 3764 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0588 HAL_0020 /y1986/m01/d03 table 3765 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0588 HAL_0020 /y1986/m01/d03 table 3766 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0588 HAL_0020 /y1986/m01/d03 table 3767 Used their k's and errors in k to predict dM
for single star entry, averaged this with dM
from 1/6/86, 60106, to get dM, error(dM)
pflx0594 HAL_0020 /y1986/m01/d06/h12 table 3813 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0594 HAL_0020 /y1986/m01/d06/h12 table 3814 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0594 HAL_0020 /y1986/m01/d06/h12 table 3815 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0594 HAL_0020 /y1986/m01/d06/h12 table 3816 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0594 HAL_0020 /y1986/m01/d06/h12 table 3817 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0594 HAL_0020 /y1986/m01/d06/h12 table 3818 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0594 HAL_0020 /y1986/m01/d06/h12 table 3819 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0594 HAL_0020 /y1986/m01/d06/h12 table 3820 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0595 HAL_0020 /y1986/m01/d06/h12 table 3821 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0595 HAL_0020 /y1986/m01/d06/h12 table 3822 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0595 HAL_0020 /y1986/m01/d06/h12 table 3823 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0595 HAL_0020 /y1986/m01/d06/h12 table 3824 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0595 HAL_0020 /y1986/m01/d06/h12 table 3825 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0595 HAL_0020 /y1986/m01/d06/h12 table 3826 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0595 HAL_0020 /y1986/m01/d06/h12 table 3827 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0595 HAL_0020 /y1986/m01/d06/h12 table 3828 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0601 HAL_0020 /y1986/m01/d07/h12 table 3855 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0601 HAL_0020 /y1986/m01/d07/h12 table 3856 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0601 HAL_0020 /y1986/m01/d07/h12 table 3857 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0601 HAL_0020 /y1986/m01/d07/h12 table 3858 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0601 HAL_0020 /y1986/m01/d07/h12 table 3859 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0601 HAL_0020 /y1986/m01/d07/h12 table 3860 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0601 HAL_0020 /y1986/m01/d07/h12 table 3861 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0601 HAL_0020 /y1986/m01/d07/h12 table 3862 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0602 HAL_0020 /y1986/m01/d07/h12 table 3863 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0602 HAL_0020 /y1986/m01/d07/h12 table 3864 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0602 HAL_0020 /y1986/m01/d07/h12 table 3865 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0602 HAL_0020 /y1986/m01/d07/h12 table 3866 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0602 HAL_0020 /y1986/m01/d07/h12 table 3867 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0602 HAL_0020 /y1986/m01/d07/h12 table 3868 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0602 HAL_0020 /y1986/m01/d07/h12 table 3869 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0602 HAL_0020 /y1986/m01/d07/h12 table 3870 Used HD3379 and HD25680 with PHOTOM* X's to
calc k separately, then mean and sdev to get
k, error(k), used these k's to predict dM for
each star entry, then mean and sdev to get dM,
error(dM)
pflx0621 HAL_0020 /y1986/m01/d11/h12 table 4010 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0621 HAL_0020 /y1986/m01/d11/h12 table 4011 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0621 HAL_0020 /y1986/m01/d11/h12 table 4012 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0621 HAL_0020 /y1986/m01/d11/h12 table 4013 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0621 HAL_0020 /y1986/m01/d11/h12 table 4014 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0621 HAL_0020 /y1986/m01/d11/h12 table 4015 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0621 HAL_0020 /y1986/m01/d11/h12 table 4016 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0621 HAL_0020 /y1986/m01/d11/h12 table 4017 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0622 HAL_0020 /y1986/m01/d11/h12 table 4018 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0622 HAL_0020 /y1986/m01/d11/h12 table 4019 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0622 HAL_0020 /y1986/m01/d11/h12 table 4020 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0622 HAL_0020 /y1986/m01/d11/h12 table 4021 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0622 HAL_0020 /y1986/m01/d11/h12 table 4022 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0622 HAL_0020 /y1986/m01/d11/h12 table 4023 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0622 HAL_0020 /y1986/m01/d11/h12 table 4024 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0622 HAL_0020 /y1986/m01/d11/h12 table 4025 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0623 HAL_0020 /y1986/m01/d14 table 4026 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0623 HAL_0020 /y1986/m01/d14 table 4027 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0623 HAL_0020 /y1986/m01/d14 table 4028 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0623 HAL_0020 /y1986/m01/d14 table 4029 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0623 HAL_0020 /y1986/m01/d14 table 4030 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0623 HAL_0020 /y1986/m01/d14 table 4031 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0623 HAL_0020 /y1986/m01/d14 table 4032 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0623 HAL_0020 /y1986/m01/d14 table 4033 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0624 HAL_0020 /y1986/m01/d14 table 4034 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0624 HAL_0020 /y1986/m01/d14 table 4035 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0624 HAL_0020 /y1986/m01/d14 table 4036 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0624 HAL_0020 /y1986/m01/d14 table 4037 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0624 HAL_0020 /y1986/m01/d14 table 4038 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0624 HAL_0020 /y1986/m01/d14 table 4039 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0624 HAL_0020 /y1986/m01/d14 table 4040 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0624 HAL_0020 /y1986/m01/d14 table 4041 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0625 HAL_0020 /y1986/m01/d14 table 4042 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0625 HAL_0020 /y1986/m01/d14 table 4043 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0625 HAL_0020 /y1986/m01/d14 table 4044 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0625 HAL_0020 /y1986/m01/d14 table 4045 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0625 HAL_0020 /y1986/m01/d14 table 4046 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0625 HAL_0020 /y1986/m01/d14 table 4047 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0625 HAL_0020 /y1986/m01/d14 table 4048 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0625 HAL_0020 /y1986/m01/d14 table 4049 Used their k's to calculate dM for each star
entry, then used mean and sdev to get dM and
error(dM), used their error(k)
pflx0631 HAL_0020 /y1986/m01/d18 table 4083 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0631 HAL_0020 /y1986/m01/d18 table 4085 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0631 HAL_0020 /y1986/m01/d18 table 4087 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0631 HAL_0020 /y1986/m01/d18 table 4088 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0631 HAL_0020 /y1986/m01/d18 table 4089 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0631 HAL_0020 /y1986/m01/d18 table 4091 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0631 HAL_0020 /y1986/m01/d18 table 4092 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0631 HAL_0020 /y1986/m01/d18 table 4093 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0632 HAL_0020 /y1986/m01/d18 table 4096 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0632 HAL_0020 /y1986/m01/d18 table 4098 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0632 HAL_0020 /y1986/m01/d18 table 4099 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0632 HAL_0020 /y1986/m01/d18 table 4100 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0632 HAL_0020 /y1986/m01/d18 table 4101 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0632 HAL_0020 /y1986/m01/d18 table 4103 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0632 HAL_0020 /y1986/m01/d18 table 4104 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0632 HAL_0020 /y1986/m01/d18 table 4105 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0799 HAL_0021 /y1986/m03/d22/h00 table 5349 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0799 HAL_0021 /y1986/m03/d22/h00 table 5350 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0799 HAL_0021 /y1986/m03/d22/h00 table 5351 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0799 HAL_0021 /y1986/m03/d22/h00 table 5352 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0799 HAL_0021 /y1986/m03/d22/h00 table 5353 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0799 HAL_0021 /y1986/m03/d22/h00 table 5354 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0799 HAL_0021 /y1986/m03/d22/h00 table 5355 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0799 HAL_0021 /y1986/m03/d22/h00 table 5356 Fits are nice so just used k's and dM's from
combined fit to HD3379 and HD219188 using
PHOTOM* X's
pflx0868 HAL_0021 /y1986/m03/d28 table 5823 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0868 HAL_0021 /y1986/m03/d28 table 5824 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0868 HAL_0021 /y1986/m03/d28 table 5825 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0868 HAL_0021 /y1986/m03/d28 table 5826 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0868 HAL_0021 /y1986/m03/d28 table 5827 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0868 HAL_0021 /y1986/m03/d28 table 5828 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0868 HAL_0021 /y1986/m03/d28 table 5829 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0869 HAL_0021 /y1986/m03/d29 table 5830 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0869 HAL_0021 /y1986/m03/d29 table 5831 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0869 HAL_0021 /y1986/m03/d29 table 5832 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0869 HAL_0021 /y1986/m03/d29 table 5833 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0869 HAL_0021 /y1986/m03/d29 table 5834 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0869 HAL_0021 /y1986/m03/d29 table 5835 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0869 HAL_0021 /y1986/m03/d29 table 5836 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx0869 HAL_0021 /y1986/m03/d29 table 5837 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/21/86, 60321, to get error(dM), used their
error(k)
pflx1918 HAL_0022 /y1986/m04/d16/h12 table 14103 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/28/86, 60328, to get error(dM), used their
error(k)
pflx1918 HAL_0022 /y1986/m04/d16/h12 table 14104 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/28/86, 60328, to get error(dM), used their
error(k)
pflx1918 HAL_0022 /y1986/m04/d16/h12 table 14105 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/28/86, 60328, to get error(dM), used their
error(k)
pflx1918 HAL_0022 /y1986/m04/d16/h12 table 14106 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/28/86, 60328, to get error(dM), used their
error(k)
pflx1918 HAL_0022 /y1986/m04/d16/h12 table 14107 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/28/86, 60328, to get error(dM), used their
error(k)
pflx1918 HAL_0022 /y1986/m04/d16/h12 table 14108 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/28/86, 60328, to get error(dM), used their
error(k)
pflx1918 HAL_0022 /y1986/m04/d16/h12 table 14109 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/28/86, 60328, to get error(dM), used their
error(k)
pflx1918 HAL_0022 /y1986/m04/d16/h12 table 14110 Used their k's to predict dM for single star
entry, used half difference with dM's from
3/28/86, 60328, to get error(dM), used their
error(k)
pflx2024 HAL_0022 /y1986/m04/d29/h12 table 14927 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2024 HAL_0022 /y1986/m04/d29/h12 table 14928 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2024 HAL_0022 /y1986/m04/d29/h12 table 14929 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2024 HAL_0022 /y1986/m04/d29/h12 table 14930 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2024 HAL_0022 /y1986/m04/d29/h12 table 14931 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2024 HAL_0022 /y1986/m04/d29/h12 table 14932 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2024 HAL_0022 /y1986/m04/d29/h12 table 14933 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2024 HAL_0022 /y1986/m04/d29/h12 table 14934 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2025 HAL_0022 /y1986/m04/d29/h12 table 14935 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2025 HAL_0022 /y1986/m04/d29/h12 table 14936 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2025 HAL_0022 /y1986/m04/d29/h12 table 14937 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2025 HAL_0022 /y1986/m04/d29/h12 table 14938 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2025 HAL_0022 /y1986/m04/d29/h12 table 14939 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2025 HAL_0022 /y1986/m04/d29/h12 table 14940 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2025 HAL_0022 /y1986/m04/d29/h12 table 14941 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2025 HAL_0022 /y1986/m04/d29/h12 table 14942 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2026 HAL_0022 /y1986/m04/d29/h12 table 14943 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2026 HAL_0022 /y1986/m04/d29/h12 table 14944 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2026 HAL_0022 /y1986/m04/d29/h12 table 14945 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2026 HAL_0022 /y1986/m04/d29/h12 table 14946 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2026 HAL_0022 /y1986/m04/d29/h12 table 14947 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2026 HAL_0022 /y1986/m04/d29/h12 table 14948 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2026 HAL_0022 /y1986/m04/d29/h12 table 14949 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2026 HAL_0022 /y1986/m04/d29/h12 table 14950 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2036 HAL_0022 /y1986/m04/d30/h12 table 15005 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2036 HAL_0022 /y1986/m04/d30/h12 table 15006 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2036 HAL_0022 /y1986/m04/d30/h12 table 15007 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2036 HAL_0022 /y1986/m04/d30/h12 table 15008 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2036 HAL_0022 /y1986/m04/d30/h12 table 15009 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2036 HAL_0022 /y1986/m04/d30/h12 table 15010 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2036 HAL_0022 /y1986/m04/d30/h12 table 15011 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2036 HAL_0022 /y1986/m04/d30/h12 table 15012 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2037 HAL_0022 /y1986/m04/d30/h12 table 15013 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2037 HAL_0022 /y1986/m04/d30/h12 table 15014 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2037 HAL_0022 /y1986/m04/d30/h12 table 15015 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2037 HAL_0022 /y1986/m04/d30/h12 table 15016 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2037 HAL_0022 /y1986/m04/d30/h12 table 15017 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2037 HAL_0022 /y1986/m04/d30/h12 table 15018 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2037 HAL_0022 /y1986/m04/d30/h12 table 15019 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2037 HAL_0022 /y1986/m04/d30/h12 table 15020 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2038 HAL_0022 /y1986/m04/d30/h12 table 15021 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2038 HAL_0022 /y1986/m04/d30/h12 table 15022 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2038 HAL_0022 /y1986/m04/d30/h12 table 15023 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2038 HAL_0022 /y1986/m04/d30/h12 table 15024 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2038 HAL_0022 /y1986/m04/d30/h12 table 15025 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2038 HAL_0022 /y1986/m04/d30/h12 table 15026 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2038 HAL_0022 /y1986/m04/d30/h12 table 15027 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2038 HAL_0022 /y1986/m04/d30/h12 table 15028 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2039 HAL_0022 /y1986/m04/d30/h12 table 15029 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2039 HAL_0022 /y1986/m04/d30/h12 table 15030 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2039 HAL_0022 /y1986/m04/d30/h12 table 15031 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2039 HAL_0022 /y1986/m04/d30/h12 table 15032 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2039 HAL_0022 /y1986/m04/d30/h12 table 15033 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2039 HAL_0022 /y1986/m04/d30/h12 table 15034 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2039 HAL_0022 /y1986/m04/d30/h12 table 15035 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2039 HAL_0022 /y1986/m04/d30/h12 table 15036 Used their k's to predict dM for each star
entry, used mean and sdev to get dM and
error(dM), used their error(k)
pflx2040 HAL_0022 /y1986/m05/d01/h00 table 15037 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2040 HAL_0022 /y1986/m05/d01/h00 table 15038 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2040 HAL_0022 /y1986/m05/d01/h00 table 15039 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2040 HAL_0022 /y1986/m05/d01/h00 table 15040 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2040 HAL_0022 /y1986/m05/d01/h00 table 15041 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2040 HAL_0022 /y1986/m05/d01/h00 table 15042 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2041 HAL_0022 /y1986/m05/d01/h00 table 15043 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2041 HAL_0022 /y1986/m05/d01/h00 table 15044 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2041 HAL_0022 /y1986/m05/d01/h00 table 15045 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2041 HAL_0022 /y1986/m05/d01/h00 table 15046 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2041 HAL_0022 /y1986/m05/d01/h00 table 15047 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2041 HAL_0022 /y1986/m05/d01/h00 table 15048 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2041 HAL_0022 /y1986/m05/d01/h00 table 15049 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2042 HAL_0022 /y1986/m05/d01/h00 table 15050 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2042 HAL_0022 /y1986/m05/d01/h00 table 15051 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2042 HAL_0022 /y1986/m05/d01/h00 table 15052 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2042 HAL_0022 /y1986/m05/d01/h00 table 15053 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2042 HAL_0022 /y1986/m05/d01/h00 table 15054 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2043 HAL_0022 /y1986/m05/d01/h00 table 15055 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2043 HAL_0022 /y1986/m05/d01/h00 table 15056 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2043 HAL_0022 /y1986/m05/d01/h00 table 15057 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2043 HAL_0022 /y1986/m05/d01/h00 table 15058 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2043 HAL_0022 /y1986/m05/d01/h00 table 15059 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2043 HAL_0022 /y1986/m05/d01/h00 table 15060 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2044 HAL_0022 /y1986/m05/d01/h00 table 15061 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2044 HAL_0022 /y1986/m05/d01/h00 table 15062 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2044 HAL_0022 /y1986/m05/d01/h00 table 15063 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2044 HAL_0022 /y1986/m05/d01/h00 table 15064 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2044 HAL_0022 /y1986/m05/d01/h00 table 15065 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2044 HAL_0022 /y1986/m05/d01/h00 table 15066 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2045 HAL_0022 /y1986/m05/d01/h00 table 15067 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2045 HAL_0022 /y1986/m05/d01/h00 table 15068 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2045 HAL_0022 /y1986/m05/d01/h00 table 15069 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2045 HAL_0022 /y1986/m05/d01/h00 table 15070 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2045 HAL_0022 /y1986/m05/d01/h00 table 15071 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2045 HAL_0022 /y1986/m05/d01/h00 table 15072 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2046 HAL_0022 /y1986/m05/d01/h00 table 15073 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2046 HAL_0022 /y1986/m05/d01/h00 table 15074 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2046 HAL_0022 /y1986/m05/d01/h00 table 15075 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2046 HAL_0022 /y1986/m05/d01/h00 table 15076 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers.
pflx2047 HAL_0022 /y1986/m05/d01/h00 table 15077 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2047 HAL_0022 /y1986/m05/d01/h00 table 15080 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2047 HAL_0022 /y1986/m05/d01/h00 table 15081 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2047 HAL_0022 /y1986/m05/d01/h00 table 15082 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2047 HAL_0022 /y1986/m05/d01/h00 table 15083 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2047 HAL_0022 /y1986/m05/d01/h00 table 15084 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2047 HAL_0022 /y1986/m05/d01/h00 table 15085 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2047 HAL_0022 /y1986/m05/d01/h00 table 15086 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2048 HAL_0022 /y1986/m05/d01/h00 table 15087 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2048 HAL_0022 /y1986/m05/d01/h00 table 15088 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2048 HAL_0022 /y1986/m05/d01/h00 table 15089 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2048 HAL_0022 /y1986/m05/d01/h00 table 15090 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2048 HAL_0022 /y1986/m05/d01/h00 table 15091 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2048 HAL_0022 /y1986/m05/d01/h00 table 15092 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2048 HAL_0022 /y1986/m05/d01/h00 table 15093 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2048 HAL_0022 /y1986/m05/d01/h00 table 15094 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2049 HAL_0022 /y1986/m05/d01/h00 table 15095 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2049 HAL_0022 /y1986/m05/d01/h00 table 15096 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2049 HAL_0022 /y1986/m05/d01/h00 table 15097 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2049 HAL_0022 /y1986/m05/d01/h00 table 15098 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2049 HAL_0022 /y1986/m05/d01/h00 table 15099 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2049 HAL_0022 /y1986/m05/d01/h00 table 15100 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2049 HAL_0022 /y1986/m05/d01/h00 table 15101 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2049 HAL_0022 /y1986/m05/d01/h00 table 15102 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2050 HAL_0022 /y1986/m05/d01/h00 table 15103 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2050 HAL_0022 /y1986/m05/d01/h00 table 15104 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2050 HAL_0022 /y1986/m05/d01/h00 table 15105 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2050 HAL_0022 /y1986/m05/d01/h00 table 15106 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2050 HAL_0022 /y1986/m05/d01/h00 table 15107 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2050 HAL_0022 /y1986/m05/d01/h00 table 15108 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2050 HAL_0022 /y1986/m05/d01/h00 table 15109 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2050 HAL_0022 /y1986/m05/d01/h00 table 15110 There are extra Tarija fluxes from this night,
1986May01. They are located in the
idxunix.52extra file and have made up catalog
numbers. Supplemented m0 data with other stars
(see "m0x" file). Fits are excellent. Used k's
and dM's from simultaneous fit with PHOTOM*.
pflx2059 HAL_0022 /y1986/m05/d02/h00 table 15168 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2059 HAL_0022 /y1986/m05/d02/h00 table 15170 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2059 HAL_0022 /y1986/m05/d02/h00 table 15171 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2059 HAL_0022 /y1986/m05/d02/h00 table 15172 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2059 HAL_0022 /y1986/m05/d02/h00 table 15173 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2059 HAL_0022 /y1986/m05/d02/h00 table 15174 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2059 HAL_0022 /y1986/m05/d02/h00 table 15175 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2059 HAL_0022 /y1986/m05/d02/h00 table 15176 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2062 HAL_0022 /y1986/m05/d02/h00 table 15189 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2062 HAL_0022 /y1986/m05/d02/h00 table 15190 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2062 HAL_0022 /y1986/m05/d02/h00 table 15191 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2062 HAL_0022 /y1986/m05/d02/h00 table 15192 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2062 HAL_0022 /y1986/m05/d02/h00 table 15193 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2062 HAL_0022 /y1986/m05/d02/h00 table 15194 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2062 HAL_0022 /y1986/m05/d02/h00 table 15195 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2062 HAL_0022 /y1986/m05/d02/h00 table 15196 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2063 HAL_0022 /y1986/m05/d02/h00 table 15197 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2063 HAL_0022 /y1986/m05/d02/h00 table 15198 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2063 HAL_0022 /y1986/m05/d02/h00 table 15199 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2063 HAL_0022 /y1986/m05/d02/h00 table 15200 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2063 HAL_0022 /y1986/m05/d02/h00 table 15201 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2063 HAL_0022 /y1986/m05/d02/h00 table 15202 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2063 HAL_0022 /y1986/m05/d02/h00 table 15203 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2063 HAL_0022 /y1986/m05/d02/h00 table 15204 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2064 HAL_0022 /y1986/m05/d02/h00 table 15205 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2064 HAL_0022 /y1986/m05/d02/h00 table 15206 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2064 HAL_0022 /y1986/m05/d02/h00 table 15207 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2064 HAL_0022 /y1986/m05/d02/h00 table 15208 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2064 HAL_0022 /y1986/m05/d02/h00 table 15209 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2064 HAL_0022 /y1986/m05/d02/h00 table 15210 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2064 HAL_0022 /y1986/m05/d02/h00 table 15211 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2064 HAL_0022 /y1986/m05/d02/h00 table 15212 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2065 HAL_0022 /y1986/m05/d02/h00 table 15213 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2065 HAL_0022 /y1986/m05/d02/h00 table 15214 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2065 HAL_0022 /y1986/m05/d02/h00 table 15215 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2065 HAL_0022 /y1986/m05/d02/h00 table 15216 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2065 HAL_0022 /y1986/m05/d02/h00 table 15217 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2065 HAL_0022 /y1986/m05/d02/h00 table 15218 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2065 HAL_0022 /y1986/m05/d02/h00 table 15219 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2065 HAL_0022 /y1986/m05/d02/h00 table 15220 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2066 HAL_0022 /y1986/m05/d02/h00 table 15221 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2066 HAL_0022 /y1986/m05/d02/h00 table 15222 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2066 HAL_0022 /y1986/m05/d02/h00 table 15223 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2066 HAL_0022 /y1986/m05/d02/h00 table 15224 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2066 HAL_0022 /y1986/m05/d02/h00 table 15225 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2066 HAL_0022 /y1986/m05/d02/h00 table 15226 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2066 HAL_0022 /y1986/m05/d02/h00 table 15227 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2066 HAL_0022 /y1986/m05/d02/h00 table 15228 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2067 HAL_0022 /y1986/m05/d02/h00 table 15229 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2067 HAL_0022 /y1986/m05/d02/h00 table 15230 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2067 HAL_0022 /y1986/m05/d02/h00 table 15231 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2067 HAL_0022 /y1986/m05/d02/h00 table 15232 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2067 HAL_0022 /y1986/m05/d02/h00 table 15233 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2067 HAL_0022 /y1986/m05/d02/h00 table 15234 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2067 HAL_0022 /y1986/m05/d02/h00 table 15235 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2067 HAL_0022 /y1986/m05/d02/h00 table 15236 Supplemented m0 data with other stars (see "imx"
file). Used PHOTOM* to calculate k's and dM's
for east and west separately. dM seems to be
different for east and west sides of the meridian.
-Missing continuous mag 6840 and 5140- (PHOTOM*
omitted data from this set).
pflx2071 HAL_0022 /y1986/m05/d03/h00 table 15252 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2071 HAL_0022 /y1986/m05/d03/h00 table 15253 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2071 HAL_0022 /y1986/m05/d03/h00 table 15254 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2071 HAL_0022 /y1986/m05/d03/h00 table 15255 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2071 HAL_0022 /y1986/m05/d03/h00 table 15256 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2071 HAL_0022 /y1986/m05/d03/h00 table 15257 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2071 HAL_0022 /y1986/m05/d03/h00 table 15258 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2071 HAL_0022 /y1986/m05/d03/h00 table 15259 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2072 HAL_0022 /y1986/m05/d03/h00 table 15260 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2072 HAL_0022 /y1986/m05/d03/h00 table 15261 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2072 HAL_0022 /y1986/m05/d03/h00 table 15262 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2072 HAL_0022 /y1986/m05/d03/h00 table 15263 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2072 HAL_0022 /y1986/m05/d03/h00 table 15264 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2072 HAL_0022 /y1986/m05/d03/h00 table 15265 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2072 HAL_0022 /y1986/m05/d03/h00 table 15266 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2072 HAL_0022 /y1986/m05/d03/h00 table 15267 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2073 HAL_0022 /y1986/m05/d03/h00 table 15268 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2073 HAL_0022 /y1986/m05/d03/h00 table 15269 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2073 HAL_0022 /y1986/m05/d03/h00 table 15270 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2073 HAL_0022 /y1986/m05/d03/h00 table 15271 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2073 HAL_0022 /y1986/m05/d03/h00 table 15272 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2073 HAL_0022 /y1986/m05/d03/h00 table 15273 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2073 HAL_0022 /y1986/m05/d03/h00 table 15274 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2073 HAL_0022 /y1986/m05/d03/h00 table 15275 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2074 HAL_0022 /y1986/m05/d03/h00 table 15276 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2074 HAL_0022 /y1986/m05/d03/h00 table 15277 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2074 HAL_0022 /y1986/m05/d03/h00 table 15278 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2074 HAL_0022 /y1986/m05/d03/h00 table 15279 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2074 HAL_0022 /y1986/m05/d03/h00 table 15280 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2074 HAL_0022 /y1986/m05/d03/h00 table 15281 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2074 HAL_0022 /y1986/m05/d03/h00 table 15282 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2074 HAL_0022 /y1986/m05/d03/h00 table 15283 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2075 HAL_0022 /y1986/m05/d03/h00 table 15284 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2075 HAL_0022 /y1986/m05/d03/h00 table 15285 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2075 HAL_0022 /y1986/m05/d03/h00 table 15286 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2075 HAL_0022 /y1986/m05/d03/h00 table 15287 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2075 HAL_0022 /y1986/m05/d03/h00 table 15288 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2075 HAL_0022 /y1986/m05/d03/h00 table 15289 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2075 HAL_0022 /y1986/m05/d03/h00 table 15290 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2075 HAL_0022 /y1986/m05/d03/h00 table 15291 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2076 HAL_0022 /y1986/m05/d03/h00 table 15292 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2076 HAL_0022 /y1986/m05/d03/h00 table 15293 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2076 HAL_0022 /y1986/m05/d03/h00 table 15294 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2076 HAL_0022 /y1986/m05/d03/h00 table 15295 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2076 HAL_0022 /y1986/m05/d03/h00 table 15296 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2076 HAL_0022 /y1986/m05/d03/h00 table 15297 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2076 HAL_0022 /y1986/m05/d03/h00 table 15298 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2076 HAL_0022 /y1986/m05/d03/h00 table 15299 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2077 HAL_0022 /y1986/m05/d03/h00 table 15300 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2077 HAL_0022 /y1986/m05/d03/h00 table 15301 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2077 HAL_0022 /y1986/m05/d03/h00 table 15302 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2077 HAL_0022 /y1986/m05/d03/h00 table 15303 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2077 HAL_0022 /y1986/m05/d03/h00 table 15304 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2077 HAL_0022 /y1986/m05/d03/h00 table 15305 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2077 HAL_0022 /y1986/m05/d03/h00 table 15306 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2077 HAL_0022 /y1986/m05/d03/h00 table 15307 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2078 HAL_0022 /y1986/m05/d03/h00 table 15308 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2078 HAL_0022 /y1986/m05/d03/h00 table 15309 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2078 HAL_0022 /y1986/m05/d03/h00 table 15310 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2078 HAL_0022 /y1986/m05/d03/h00 table 15311 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2078 HAL_0022 /y1986/m05/d03/h00 table 15312 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2078 HAL_0022 /y1986/m05/d03/h00 table 15313 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2078 HAL_0022 /y1986/m05/d03/h00 table 15314 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2078 HAL_0022 /y1986/m05/d03/h00 table 15315 Added 2 IMX stars and used simultaneous fit from
PHOTOM*
pflx2088 HAL_0022 /y1986/m05/d05 table 15405 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2088 HAL_0022 /y1986/m05/d05 table 15406 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2088 HAL_0022 /y1986/m05/d05 table 15407 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2088 HAL_0022 /y1986/m05/d05 table 15408 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2088 HAL_0022 /y1986/m05/d05 table 15409 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2088 HAL_0022 /y1986/m05/d05 table 15410 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2088 HAL_0022 /y1986/m05/d05 table 15411 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2088 HAL_0022 /y1986/m05/d05 table 15412 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2089 HAL_0022 /y1986/m05/d05 table 15413 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2089 HAL_0022 /y1986/m05/d05 table 15414 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2089 HAL_0022 /y1986/m05/d05 table 15415 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2089 HAL_0022 /y1986/m05/d05 table 15416 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2089 HAL_0022 /y1986/m05/d05 table 15417 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2089 HAL_0022 /y1986/m05/d05 table 15418 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2089 HAL_0022 /y1986/m05/d05 table 15419 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2089 HAL_0022 /y1986/m05/d05 table 15420 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2090 HAL_0022 /y1986/m05/d05 table 15421 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2090 HAL_0022 /y1986/m05/d05 table 15422 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2090 HAL_0022 /y1986/m05/d05 table 15423 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2090 HAL_0022 /y1986/m05/d05 table 15424 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2090 HAL_0022 /y1986/m05/d05 table 15425 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2090 HAL_0022 /y1986/m05/d05 table 15426 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2090 HAL_0022 /y1986/m05/d05 table 15427 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2090 HAL_0022 /y1986/m05/d05 table 15428 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2091 HAL_0022 /y1986/m05/d05 table 15429 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2091 HAL_0022 /y1986/m05/d05 table 15430 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2091 HAL_0022 /y1986/m05/d05 table 15431 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2091 HAL_0022 /y1986/m05/d05 table 15432 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2091 HAL_0022 /y1986/m05/d05 table 15433 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2091 HAL_0022 /y1986/m05/d05 table 15434 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2091 HAL_0022 /y1986/m05/d05 table 15435 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2091 HAL_0022 /y1986/m05/d05 table 15436 Used k's and error(k)'s from 4/29/86, 60429,
estimated dM for single star entry, then
estimated error(dM) as half difference to
4/30/86, 60430, dM's
pflx2107 HAL_0022 /y1986/m05/d06/h00 table 15530 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2107 HAL_0022 /y1986/m05/d06/h00 table 15531 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2107 HAL_0022 /y1986/m05/d06/h00 table 15532 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2107 HAL_0022 /y1986/m05/d06/h00 table 15533 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2107 HAL_0022 /y1986/m05/d06/h00 table 15534 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2107 HAL_0022 /y1986/m05/d06/h00 table 15535 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2107 HAL_0022 /y1986/m05/d06/h00 table 15536 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2107 HAL_0022 /y1986/m05/d06/h00 table 15537 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2108 HAL_0022 /y1986/m05/d06/h00 table 15538 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2108 HAL_0022 /y1986/m05/d06/h00 table 15539 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2108 HAL_0022 /y1986/m05/d06/h00 table 15540 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2108 HAL_0022 /y1986/m05/d06/h00 table 15541 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2108 HAL_0022 /y1986/m05/d06/h00 table 15542 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2108 HAL_0022 /y1986/m05/d06/h00 table 15543 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2108 HAL_0022 /y1986/m05/d06/h00 table 15544 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2108 HAL_0022 /y1986/m05/d06/h00 table 15545 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2110 HAL_0022 /y1986/m05/d06/h00 table 15551 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2110 HAL_0022 /y1986/m05/d06/h00 table 15553 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2110 HAL_0022 /y1986/m05/d06/h00 table 15555 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2110 HAL_0022 /y1986/m05/d06/h00 table 15556 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2110 HAL_0022 /y1986/m05/d06/h00 table 15558 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2110 HAL_0022 /y1986/m05/d06/h00 table 15559 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2110 HAL_0022 /y1986/m05/d06/h00 table 15560 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2110 HAL_0022 /y1986/m05/d06/h00 table 15561 Comet is only west in the sky, all stars are
west, used simultaneous fit from PHOTOM*
pflx2182 HAL_0022 /y1986/m05/d07/h12 table 16088 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2182 HAL_0022 /y1986/m05/d07/h12 table 16089 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2182 HAL_0022 /y1986/m05/d07/h12 table 16090 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2182 HAL_0022 /y1986/m05/d07/h12 table 16091 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2182 HAL_0022 /y1986/m05/d07/h12 table 16092 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2182 HAL_0022 /y1986/m05/d07/h12 table 16093 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2182 HAL_0022 /y1986/m05/d07/h12 table 16094 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2182 HAL_0022 /y1986/m05/d07/h12 table 16095 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2183 HAL_0022 /y1986/m05/d08/h00 table 16096 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2183 HAL_0022 /y1986/m05/d08/h00 table 16097 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2183 HAL_0022 /y1986/m05/d08/h00 table 16098 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2183 HAL_0022 /y1986/m05/d08/h00 table 16099 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2183 HAL_0022 /y1986/m05/d08/h00 table 16100 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2183 HAL_0022 /y1986/m05/d08/h00 table 16101 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2183 HAL_0022 /y1986/m05/d08/h00 table 16102 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2183 HAL_0022 /y1986/m05/d08/h00 table 16103 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2184 HAL_0022 /y1986/m05/d08/h00 table 16104 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2184 HAL_0022 /y1986/m05/d08/h00 table 16105 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2184 HAL_0022 /y1986/m05/d08/h00 table 16106 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2184 HAL_0022 /y1986/m05/d08/h00 table 16107 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2184 HAL_0022 /y1986/m05/d08/h00 table 16109 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2184 HAL_0022 /y1986/m05/d08/h00 table 16111 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2184 HAL_0022 /y1986/m05/d08/h00 table 16121 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2184 HAL_0022 /y1986/m05/d08/h00 table 16129 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2193 HAL_0022 /y1986/m05/d08/h00 table 16175 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2193 HAL_0022 /y1986/m05/d08/h00 table 16178 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2193 HAL_0022 /y1986/m05/d08/h00 table 16179 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2193 HAL_0022 /y1986/m05/d08/h00 table 16181 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2193 HAL_0022 /y1986/m05/d08/h00 table 16182 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2193 HAL_0022 /y1986/m05/d08/h00 table 16184 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2193 HAL_0022 /y1986/m05/d08/h00 table 16186 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2195 HAL_0022 /y1986/m05/d08/h00 table 16192 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2195 HAL_0022 /y1986/m05/d08/h00 table 16193 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2195 HAL_0022 /y1986/m05/d08/h00 table 16194 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2195 HAL_0022 /y1986/m05/d08/h00 table 16195 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2195 HAL_0022 /y1986/m05/d08/h00 table 16196 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2195 HAL_0022 /y1986/m05/d08/h00 table 16197 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2195 HAL_0022 /y1986/m05/d08/h00 table 16198 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2195 HAL_0022 /y1986/m05/d08/h00 table 16199 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2197 HAL_0022 /y1986/m05/d08/h00 table 16207 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2197 HAL_0022 /y1986/m05/d08/h00 table 16209 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2197 HAL_0022 /y1986/m05/d08/h00 table 16210 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2197 HAL_0022 /y1986/m05/d08/h00 table 16211 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2197 HAL_0022 /y1986/m05/d08/h00 table 16212 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2197 HAL_0022 /y1986/m05/d08/h00 table 16213 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2197 HAL_0022 /y1986/m05/d08/h00 table 16214 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2197 HAL_0022 /y1986/m05/d08/h00 table 16215 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2199 HAL_0022 /y1986/m05/d08/h00 table 16219 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2199 HAL_0022 /y1986/m05/d08/h00 table 16221 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2199 HAL_0022 /y1986/m05/d08/h00 table 16223 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2199 HAL_0022 /y1986/m05/d08/h00 table 16225 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2199 HAL_0022 /y1986/m05/d08/h00 table 16227 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2199 HAL_0022 /y1986/m05/d08/h00 table 16229 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2199 HAL_0022 /y1986/m05/d08/h00 table 16230 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2199 HAL_0022 /y1986/m05/d08/h00 table 16231 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2203 HAL_0022 /y1986/m05/d08/h00 table 16256 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2203 HAL_0022 /y1986/m05/d08/h00 table 16257 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2203 HAL_0022 /y1986/m05/d08/h00 table 16258 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2203 HAL_0022 /y1986/m05/d08/h00 table 16263 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2203 HAL_0022 /y1986/m05/d08/h00 table 16267 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2203 HAL_0022 /y1986/m05/d08/h00 table 16269 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2203 HAL_0022 /y1986/m05/d08/h00 table 16270 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2203 HAL_0022 /y1986/m05/d08/h00 table 16271 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2206 HAL_0022 /y1986/m05/d08/h00 table 16280 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2206 HAL_0022 /y1986/m05/d08/h00 table 16281 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2206 HAL_0022 /y1986/m05/d08/h00 table 16282 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2206 HAL_0022 /y1986/m05/d08/h00 table 16283 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2206 HAL_0022 /y1986/m05/d08/h00 table 16284 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2206 HAL_0022 /y1986/m05/d08/h00 table 16285 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2206 HAL_0022 /y1986/m05/d08/h00 table 16286 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2206 HAL_0022 /y1986/m05/d08/h00 table 16287 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2208 HAL_0022 /y1986/m05/d08/h00 table 16292 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2208 HAL_0022 /y1986/m05/d08/h00 table 16295 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2208 HAL_0022 /y1986/m05/d08/h00 table 16298 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2208 HAL_0022 /y1986/m05/d08/h00 table 16299 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2208 HAL_0022 /y1986/m05/d08/h00 table 16300 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2208 HAL_0022 /y1986/m05/d08/h00 table 16301 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2208 HAL_0022 /y1986/m05/d08/h00 table 16302 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2208 HAL_0022 /y1986/m05/d08/h00 table 16303 Added in 3 IMX star entries. Used PHOTOM*
simultaneous fits for east stars and west
stars
pflx2252 HAL_0022 /y1986/m05/d09/h00 table 16599 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2252 HAL_0022 /y1986/m05/d09/h00 table 16600 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2252 HAL_0022 /y1986/m05/d09/h00 table 16601 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2252 HAL_0022 /y1986/m05/d09/h00 table 16602 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2252 HAL_0022 /y1986/m05/d09/h00 table 16603 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2252 HAL_0022 /y1986/m05/d09/h00 table 16604 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2252 HAL_0022 /y1986/m05/d09/h00 table 16605 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2252 HAL_0022 /y1986/m05/d09/h00 table 16606 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2253 HAL_0022 /y1986/m05/d09/h00 table 16607 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2253 HAL_0022 /y1986/m05/d09/h00 table 16608 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2253 HAL_0022 /y1986/m05/d09/h00 table 16609 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2253 HAL_0022 /y1986/m05/d09/h00 table 16610 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2253 HAL_0022 /y1986/m05/d09/h00 table 16611 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2253 HAL_0022 /y1986/m05/d09/h00 table 16612 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2253 HAL_0022 /y1986/m05/d09/h00 table 16613 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2253 HAL_0022 /y1986/m05/d09/h00 table 16614 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2254 HAL_0022 /y1986/m05/d09/h00 table 16615 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2254 HAL_0022 /y1986/m05/d09/h00 table 16616 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2254 HAL_0022 /y1986/m05/d09/h00 table 16617 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2254 HAL_0022 /y1986/m05/d09/h00 table 16618 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2254 HAL_0022 /y1986/m05/d09/h00 table 16619 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2254 HAL_0022 /y1986/m05/d09/h00 table 16620 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2254 HAL_0022 /y1986/m05/d09/h00 table 16621 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2254 HAL_0022 /y1986/m05/d09/h00 table 16622 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2256 HAL_0022 /y1986/m05/d09/h00 table 16631 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2256 HAL_0022 /y1986/m05/d09/h00 table 16632 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2256 HAL_0022 /y1986/m05/d09/h00 table 16633 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2256 HAL_0022 /y1986/m05/d09/h00 table 16634 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2256 HAL_0022 /y1986/m05/d09/h00 table 16635 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2256 HAL_0022 /y1986/m05/d09/h00 table 16636 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2256 HAL_0022 /y1986/m05/d09/h00 table 16637 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2256 HAL_0022 /y1986/m05/d09/h00 table 16638 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2257 HAL_0022 /y1986/m05/d09/h00 table 16639 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2257 HAL_0022 /y1986/m05/d09/h00 table 16640 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2257 HAL_0022 /y1986/m05/d09/h00 table 16641 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2257 HAL_0022 /y1986/m05/d09/h00 table 16642 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2257 HAL_0022 /y1986/m05/d09/h00 table 16643 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2257 HAL_0022 /y1986/m05/d09/h00 table 16644 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2257 HAL_0022 /y1986/m05/d09/h00 table 16645 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2257 HAL_0022 /y1986/m05/d09/h00 table 16646 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2258 HAL_0022 /y1986/m05/d09/h00 table 16647 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2258 HAL_0022 /y1986/m05/d09/h00 table 16648 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2258 HAL_0022 /y1986/m05/d09/h00 table 16649 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2258 HAL_0022 /y1986/m05/d09/h00 table 16650 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2258 HAL_0022 /y1986/m05/d09/h00 table 16651 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2258 HAL_0022 /y1986/m05/d09/h00 table 16652 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2258 HAL_0022 /y1986/m05/d09/h00 table 16653 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2258 HAL_0022 /y1986/m05/d09/h00 table 16654 Used PHOTOM* simultaneous fits for east stars
and for west stars
pflx2362 HAL_0022 /y1986/m05/d13 table 17452 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2362 HAL_0022 /y1986/m05/d13 table 17453 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2362 HAL_0022 /y1986/m05/d13 table 17454 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2362 HAL_0022 /y1986/m05/d13 table 17455 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2362 HAL_0022 /y1986/m05/d13 table 17456 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2362 HAL_0022 /y1986/m05/d13 table 17457 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2362 HAL_0022 /y1986/m05/d13 table 17458 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2362 HAL_0022 /y1986/m05/d13 table 17459 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2410 HAL_0022 /y1986/m05/d19 table 17775 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2410 HAL_0022 /y1986/m05/d19 table 17776 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2410 HAL_0022 /y1986/m05/d19 table 17777 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2410 HAL_0022 /y1986/m05/d19 table 17778 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2410 HAL_0022 /y1986/m05/d19 table 17779 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2410 HAL_0022 /y1986/m05/d19 table 17780 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2410 HAL_0022 /y1986/m05/d19 table 17781 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2410 HAL_0022 /y1986/m05/d19 table 17782 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2411 HAL_0022 /y1986/m05/d19 table 17783 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2411 HAL_0022 /y1986/m05/d19 table 17784 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2411 HAL_0022 /y1986/m05/d19 table 17785 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2411 HAL_0022 /y1986/m05/d19 table 17786 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2411 HAL_0022 /y1986/m05/d19 table 17787 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2411 HAL_0022 /y1986/m05/d19 table 17788 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2411 HAL_0022 /y1986/m05/d19 table 17789 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2411 HAL_0022 /y1986/m05/d19 table 17790 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2412 HAL_0022 /y1986/m05/d19 table 17791 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2412 HAL_0022 /y1986/m05/d19 table 17792 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2412 HAL_0022 /y1986/m05/d19 table 17793 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2412 HAL_0022 /y1986/m05/d19 table 17794 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2412 HAL_0022 /y1986/m05/d19 table 17795 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2412 HAL_0022 /y1986/m05/d19 table 17796 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2412 HAL_0022 /y1986/m05/d19 table 17797 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2412 HAL_0022 /y1986/m05/d19 table 17798 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2413 HAL_0022 /y1986/m05/d19 table 17799 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2413 HAL_0022 /y1986/m05/d19 table 17800 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2413 HAL_0022 /y1986/m05/d19 table 17801 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2413 HAL_0022 /y1986/m05/d19 table 17802 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2413 HAL_0022 /y1986/m05/d19 table 17803 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2413 HAL_0022 /y1986/m05/d19 table 17804 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2413 HAL_0022 /y1986/m05/d19 table 17805 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2413 HAL_0022 /y1986/m05/d19 table 17806 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2431 HAL_0022 /y1986/m05/d31 table 17955 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2431 HAL_0022 /y1986/m05/d31 table 17956 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2431 HAL_0022 /y1986/m05/d31 table 17957 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2431 HAL_0022 /y1986/m05/d31 table 17958 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2431 HAL_0022 /y1986/m05/d31 table 17959 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2431 HAL_0022 /y1986/m05/d31 table 17960 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2431 HAL_0022 /y1986/m05/d31 table 17961 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2431 HAL_0022 /y1986/m05/d31 table 17962 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2432 HAL_0022 /y1986/m05/d31 table 17963 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2432 HAL_0022 /y1986/m05/d31 table 17964 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2432 HAL_0022 /y1986/m05/d31 table 17965 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2432 HAL_0022 /y1986/m05/d31 table 17966 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2432 HAL_0022 /y1986/m05/d31 table 17967 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2432 HAL_0022 /y1986/m05/d31 table 17968 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2432 HAL_0022 /y1986/m05/d31 table 17969 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2432 HAL_0022 /y1986/m05/d31 table 17970 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2433 HAL_0022 /y1986/m05/d31 table 17971 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2433 HAL_0022 /y1986/m05/d31 table 17972 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2433 HAL_0022 /y1986/m05/d31 table 17973 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2433 HAL_0022 /y1986/m05/d31 table 17974 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2433 HAL_0022 /y1986/m05/d31 table 17975 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2433 HAL_0022 /y1986/m05/d31 table 17976 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2433 HAL_0022 /y1986/m05/d31 table 17977 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2433 HAL_0022 /y1986/m05/d31 table 17978 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2434 HAL_0022 /y1986/m05/d31 table 17979 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2434 HAL_0022 /y1986/m05/d31 table 17980 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2434 HAL_0022 /y1986/m05/d31 table 17981 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2434 HAL_0022 /y1986/m05/d31 table 17982 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2434 HAL_0022 /y1986/m05/d31 table 17983 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2434 HAL_0022 /y1986/m05/d31 table 17984 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2434 HAL_0022 /y1986/m05/d31 table 17985 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2434 HAL_0022 /y1986/m05/d31 table 17986 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2461 HAL_0022 /y1986/m06/d05 table 18182 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2461 HAL_0022 /y1986/m06/d05 table 18183 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2461 HAL_0022 /y1986/m06/d05 table 18184 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2461 HAL_0022 /y1986/m06/d05 table 18185 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2461 HAL_0022 /y1986/m06/d05 table 18186 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2461 HAL_0022 /y1986/m06/d05 table 18187 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2461 HAL_0022 /y1986/m06/d05 table 18188 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2461 HAL_0022 /y1986/m06/d05 table 18189 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2462 HAL_0022 /y1986/m06/d05 table 18190 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2462 HAL_0022 /y1986/m06/d05 table 18191 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2462 HAL_0022 /y1986/m06/d05 table 18192 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2462 HAL_0022 /y1986/m06/d05 table 18193 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2462 HAL_0022 /y1986/m06/d05 table 18194 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2462 HAL_0022 /y1986/m06/d05 table 18195 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2462 HAL_0022 /y1986/m06/d05 table 18196 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2462 HAL_0022 /y1986/m06/d05 table 18197 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2463 HAL_0022 /y1986/m06/d05 table 18198 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2463 HAL_0022 /y1986/m06/d05 table 18199 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2463 HAL_0022 /y1986/m06/d05 table 18200 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2463 HAL_0022 /y1986/m06/d05 table 18201 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2463 HAL_0022 /y1986/m06/d05 table 18202 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2463 HAL_0022 /y1986/m06/d05 table 18203 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2463 HAL_0022 /y1986/m06/d05 table 18204 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2463 HAL_0022 /y1986/m06/d05 table 18205 Used their k's to predict dM for each star
entry, then averaged these dM's and used mean
and sdev to get dM and error(dM), used their
error(k)
pflx2476 HAL_0022 /y1986/m06/d13 table 18315 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2476 HAL_0022 /y1986/m06/d13 table 18316 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2476 HAL_0022 /y1986/m06/d13 table 18317 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2476 HAL_0022 /y1986/m06/d13 table 18318 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2476 HAL_0022 /y1986/m06/d13 table 18319 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2476 HAL_0022 /y1986/m06/d13 table 18320 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2476 HAL_0022 /y1986/m06/d13 table 18321 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2476 HAL_0022 /y1986/m06/d13 table 18322 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2477 HAL_0022 /y1986/m06/d13 table 18323 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2477 HAL_0022 /y1986/m06/d13 table 18324 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2477 HAL_0022 /y1986/m06/d13 table 18325 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2477 HAL_0022 /y1986/m06/d13 table 18326 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2477 HAL_0022 /y1986/m06/d13 table 18327 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2477 HAL_0022 /y1986/m06/d13 table 18328 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2477 HAL_0022 /y1986/m06/d13 table 18329 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2477 HAL_0022 /y1986/m06/d13 table 18330 Comet was west and all star entries were west.
Everything looks okay (compared with TUN26BZ,
6/26/86, and TUN30BZ, 6/30/86) except HD89688
filters 7 and 8, so omitted them from the
PHOTOM* fit. Assumed delta_k=0.01,
delta_0.05 for filters 7 and 8
pflx2483 HAL_0022 /y1986/m06/d26 table 18368 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2483 HAL_0022 /y1986/m06/d26 table 18369 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2483 HAL_0022 /y1986/m06/d26 table 18370 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2483 HAL_0022 /y1986/m06/d26 table 18371 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2483 HAL_0022 /y1986/m06/d26 table 18372 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2483 HAL_0022 /y1986/m06/d26 table 18373 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2483 HAL_0022 /y1986/m06/d26 table 18374 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2483 HAL_0022 /y1986/m06/d26 table 18375 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2484 HAL_0022 /y1986/m06/d30 table 18376 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2484 HAL_0022 /y1986/m06/d30 table 18377 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2484 HAL_0022 /y1986/m06/d30 table 18378 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2484 HAL_0022 /y1986/m06/d30 table 18379 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2484 HAL_0022 /y1986/m06/d30 table 18380 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2484 HAL_0022 /y1986/m06/d30 table 18381 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2484 HAL_0022 /y1986/m06/d30 table 18382 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2484 HAL_0022 /y1986/m06/d30 table 18383 Comet was west and all 3 star entries were
west. Used simultaneous PHOTOM* fits
pflx2485 HAL_0022 /y1986/m07/d05 table 18384 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2485 HAL_0022 /y1986/m07/d05 table 18385 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2485 HAL_0022 /y1986/m07/d05 table 18386 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2485 HAL_0022 /y1986/m07/d05 table 18387 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2485 HAL_0022 /y1986/m07/d05 table 18388 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2485 HAL_0022 /y1986/m07/d05 table 18389 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2485 HAL_0022 /y1986/m07/d05 table 18390 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2485 HAL_0022 /y1986/m07/d05 table 18391 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2486 HAL_0022 /y1986/m07/d06 table 18392 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2486 HAL_0022 /y1986/m07/d06 table 18393 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2486 HAL_0022 /y1986/m07/d06 table 18394 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2486 HAL_0022 /y1986/m07/d06 table 18395 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2486 HAL_0022 /y1986/m07/d06 table 18396 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2486 HAL_0022 /y1986/m07/d06 table 18397 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2486 HAL_0022 /y1986/m07/d06 table 18398 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2486 HAL_0022 /y1986/m07/d06 table 18399 Used PHOTOM* simultaneous fits for 2 star
entries (different stars). Assumed
delta_k=0.01, delta_dM=0.05
pflx2487 HAL_0022 /y1986/m07/d06 table 18400 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2487 HAL_0022 /y1986/m07/d06 table 18401 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2487 HAL_0022 /y1986/m07/d06 table 18402 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2487 HAL_0022 /y1986/m07/d06 table 18403 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2487 HAL_0022 /y1986/m07/d06 table 18404 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2487 HAL_0022 /y1986/m07/d06 table 18405 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2487 HAL_0022 /y1986/m07/d06 table 18406 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2487 HAL_0022 /y1986/m07/d06 table 18407 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2488 HAL_0022 /y1986/m07/d06 table 18408 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2488 HAL_0022 /y1986/m07/d06 table 18409 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2488 HAL_0022 /y1986/m07/d06 table 18410 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2488 HAL_0022 /y1986/m07/d06 table 18411 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2488 HAL_0022 /y1986/m07/d06 table 18412 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2488 HAL_0022 /y1986/m07/d06 table 18413 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2488 HAL_0022 /y1986/m07/d06 table 18414 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2488 HAL_0022 /y1986/m07/d06 table 18415 The 3 star entries were 3 different stars,
but PHOTOM* fit seemed to be okay, so used
it
pflx2489 HAL_0022 /y1987/m01 table 18416 Used average dM from 1/5/87, 70105, and
1/6/87, 70106, and added in as another
Mi-Ms star entry for X=0, then fitted
together to get k and dM simultaneously (with
errors)
pflx2489 HAL_0022 /y1987/m01 table 18417 Used average dM from 1/5/87, 70105, and
1/6/87, 70106, and added in as another
Mi-Ms star entry for X=0, then fitted
together to get k and dM simultaneously (with
errors)
pflx2489 HAL_0022 /y1987/m01 table 18418 Used average dM from 1/5/87, 70105, and
1/6/87, 70106, and added in as another
Mi-Ms star entry for X=0, then fitted
together to get k and dM simultaneously (with
errors)
pflx2489 HAL_0022 /y1987/m01 table 18419 Used average dM from 1/5/87, 70105, and
1/6/87, 70106, and added in as another
Mi-Ms star entry for X=0, then fitted
together to get k and dM simultaneously (with
errors)
pflx2489 HAL_0022 /y1987/m01 table 18420 Used average dM from 1/5/87, 70105, and
1/6/87, 70106, and added in as another
Mi-Ms star entry for X=0, then fitted
together to get k and dM simultaneously (with
errors)
pflx2489 HAL_0022 /y1987/m01 table 18421 Used average dM from 1/5/87, 70105, and
1/6/87, 70106, and added in as another
Mi-Ms star entry for X=0, then fitted
together to get k and dM simultaneously (with
errors)
pflx2490 HAL_0022 /y1987/m01 table 18422 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2490 HAL_0022 /y1987/m01 table 18423 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2490 HAL_0022 /y1987/m01 table 18424 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2490 HAL_0022 /y1987/m01 table 18425 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2490 HAL_0022 /y1987/m01 table 18426 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2490 HAL_0022 /y1987/m01 table 18427 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2490 HAL_0022 /y1987/m01 table 18428 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2490 HAL_0022 /y1987/m01 table 18429 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2491 HAL_0022 /y1987/m01 table 18430 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2491 HAL_0022 /y1987/m01 table 18431 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2491 HAL_0022 /y1987/m01 table 18432 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2491 HAL_0022 /y1987/m01 table 18433 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2491 HAL_0022 /y1987/m01 table 18434 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2491 HAL_0022 /y1987/m01 table 18435 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
pflx2491 HAL_0022 /y1987/m01 table 18436 Calculated k separately for HD89688 and
HD105590 (omitted west entry) to get
weighted mean k and error(k), used these
k's to predict dM for each star entry, then
used mean and sdev to get dM and error(dM)
<1>26 January 1996