PDS_VERSION_ID = PDS3 RECORD_TYPE = "FIXED_LENGTH" RECORD_BYTES = 63 FILE_RECORDS = 14 ^TABLE = "PHOT_20000821.TAB" DATA_SET_ID = "DI/EAR-C-KECK1LWS-3-9P-IMAGES-PHOT-V1.0" PRODUCT_NAME = "KECK I LWS 9P PHOTOMETRY FROM 21 AUGUST 2000" PRODUCT_ID = "DI_9P_KECK1_LWS_PHOT_20000821" INSTRUMENT_HOST_NAME = "KECK I 10M TELESCOPE" INSTRUMENT_NAME = "KECK I LONG WAVELENGTH SPECTROGRAPH (IR)" TARGET_NAME = "9P/TEMPEL 1 (1867 G1)" START_TIME = 2000-08-21T10:51:19.92 STOP_TIME = 2000-08-21T15:53:05.34 PRODUCT_CREATION_TIME = 2004-12-16T23:40:00 OBJECT = TABLE INTERCHANGE_FORMAT = "ASCII" NAME = "9P PHOTOMETRY" ROWS = 14 ROW_BYTES = 63 COLUMNS = 5 DESCRIPTION = "This table contains mid-IR fluxes of comet 9P/Tempel 1 as measured by Fernandez et al. 2003 [FERNANDEZETAL2003]. Note that the entry for START_TIME of 2000-08-21T15:16:01.72 gives only the 3-sigma upper limit for the flux." OBJECT = COLUMN COLUMN_NUMBER = 1 NAME = "IMAGE_FILE_NAME" START_BYTE = 2 BYTES = 13 DATA_TYPE = "CHARACTER" FORMAT = "A13" DESCRIPTION = "The name of the reduced image for which the flux of 9P was measured." END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 2 NAME = "START_TIME" START_BYTE = 19 BYTES = 22 DATA_TYPE = "CHARACTER" FORMAT = "A22" DESCRIPTION = "The UTC time at the beginning of the image" END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 3 NAME = "FILTER_CENTER_WAVELENGTH" START_BYTE = 44 BYTES = 4 DATA_TYPE = "ASCII_REAL" FORMAT = "F4.1" UNIT = "MICROMETER" DESCRIPTION = "The center wavelength of the filter" END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 4 NAME = "FLUX" START_BYTE = 50 BYTES = 5 DATA_TYPE = "ASCII_REAL" FORMAT = "F5.1" UNIT = "MILLIJANSKY" DESCRIPTION = "The measured flux" END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 5 NAME = "FLUX_UNCERTAINTY" START_BYTE = 57 BYTES = 4 DATA_TYPE = "ASCII_REAL" FORMAT = "F4.1" UNIT = "MILLIJANSKY" DESCRIPTION = "The estimated uncertainty of the flux" END_OBJECT = COLUMN END_OBJECT = TABLE END