The following data are supplied to observers on FITS tapes:
c2hfile), and a calibration file which gives the throughput curve used in populating the photometric keywords (.
c3tfile) are included.
Further data reduction and analysis can be performed under the STScI's science data analysis software system (STSDAS). Standard routines are available, operating under IRAF, for the analysis of data for image photometry, spectral analysis, astrometry, and the generation of the calibration data files.