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   PR #    97
   This a program of six pointings at the supernova remnant Puppis A. Its
   goal is to spectrally map the entire SNR using the SIS. Stronglines of
   O VII, O VIII, Ne IX, Ne X, Mg XI, and Si XIV are detectable from this
   remnant (as indicated by the calibration observation),and the BBXRT
   spectral mapping indicate strong changes inrelative line strengths
   across the remnant.Calibration goals include: measuring the SIS
   spectral resolution below 2 keV;verification of pulse height to energy
   conversion; calibration of effectivearea by cross calibration with
   previous spectral and imaging observations;comparison of faint and
   bright mode data for a source filling the field of view.
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