PDS_VERSION_ID = PDS3 DATA_SET_ID = {"NH-X-LORRI-2-LAUNCH-V3.0", "NH-X-LORRI-3-LAUNCH-V3.0", "NH-J-LORRI-2-JUPITER-V3.0", "NH-J-LORRI-3-JUPITER-V3.0", "NH-X-LORRI-2-PLUTOCRUISE-V2.0", "NH-X-LORRI-3-PLUTOCRUISE-V2.0", "NH-P-LORRI-2-PLUTO-V3.0", "NH-P-LORRI-3-PLUTO-V3.0", "NH-X-LORRI-2-KEMCRUISE1-V2.0", "NH-X-LORRI-3-KEMCRUISE1-V2.0", "NH-X-LORRI-2-KEM1-V1.0", "NH-X-LORRI-3-KEM1-V1.0"} RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 2019-12-16 NOTE = "ERRATA.TXT reflects any known deficiencies with files contained on volume USA_NASA_SBN_NH**LO_*001." END_OBJECT = TEXT END ERRATA This file contains a list of all deficiencies and irregularities that are known to exist at the time of the publication date above. Any errors detected with this volume will be published on subsequent volumes in this volume set. All data label files and data file FITS headers: Careful analysis of LORRI raw data images reveals that the exposure time values in the FITS headers should be increased by 0.0006 seconds (0.6 ms). The preferred solution is to decrease the image start time by 0.0006 seconds, which causes a 0.0003 second shift in the image mid-time. No PDU or EDU data values are affected in either raw or calibrated data files. Since image mid-time is the base for most SPICE calculations, this change indirectly affects (in a very minor way) many values in the FITS headers and the data label files, including (but not limited to) the following: FITS Headers: STARTMET DURMET EXPTIME SPC* RATE* CD[12]_[12] CRVAL[12] PA_[XY]INST PA_SUN* SOL_ELON EAR_ELON Data Label Files: SPACECRAFT_CLOCK_START_COUNT EXPOSURE_DURATION SC_TARGET_POSITION_VECTOR TARGET_CENTER_DISTANCE TARGET_SUN_POSITION_VECTOR SOLAR_DISTANCE SC_SUN_POSITION_VECTOR SPACECRAFT_SOLAR_DISTANCE SC_EARTH_POSITION_VECTOR SC_GEOCENTRIC_DISTANCE QUATERNIONS