OBJECT = DATA_SET DATA_SET_ID = "VEGA1-C-PUMA-2-RDR-HALLEY-V1.0" OBJECT = DATA_SET_INFORMATION DATA_SET_NAME = "VEGA1 PUMA DUST MASS SPECTROMETER DATA V1.0" DATA_SET_COLLECTION_MEMBER_FLG = Y START_TIME = UNK STOP_TIME = UNK DATA_SET_RELEASE_DATE = UNK PRODUCER_FULL_NAME = "INTERNATIONAL HALLEY WATCH" DETAILED_CATALOG_FLAG = N DATA_SET_DESC = " \v Data Set Overview ================= \v The PUMA data were submitted by IKI in two unique forms, a GROUPS FITS file and undocumented binary file. In one original form, the data in this set were received as 4,027 separate FITS files, one for each spectrum. These files have been reformatted and combined into four tables, one for each of the PUMA instrument operating modes. Within each table, the spectra are in order of original FITS file number. This order is assumed to be chronological, based on time given by the BLISI clock, in sec. The second form for this original dataset was a fixed length binary file containing data taken in all instrument modes. These files were split into separate files for each mode, preserving the original ordering of the spectra within the table. Spectra in each mode table are arranged chronologically, using TIME of the spectrum on the BLISI clock, in sec. " CONFIDENCE_LEVEL_NOTE = " \v Confidence Level Overview ========================= \v N/A" END_OBJECT = DATA_SET_INFORMATION OBJECT = DATA_SET_TARGET TARGET_NAME = HALLEY END_OBJECT = DATA_SET_TARGET OBJECT = DATA_SET_HOST INSTRUMENT_HOST_ID = VEGA1 INSTRUMENT_ID = PUMA END_OBJECT = DATA_SET_HOST OBJECT = DATA_SET_REFERENCE_INFORMATION REFERENCE_KEY_ID = "ESA-SP1066" END_OBJECT = DATA_SET_REFERENCE_INFORMATION OBJECT = DATA_SET_REFERENCE_INFORMATION REFERENCE_KEY_ID = "NATURE321" END_OBJECT = DATA_SET_REFERENCE_INFORMATION END_OBJECT = DATA_SET END