FOS Cycle 3 Spectral Flat Fields and Monitor

Details FOS Cycle 3 Spectral Flat Fields and Monitor FOS Cycle 3 Spectral Flat Fields and Monitor

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.5048k&link_type=abstract

HST Proposal ID #5048

Other

Hst Proposal Id #5048

Scientific paper

Some FOS detector/disperser combinations have shown temporal variations in their flat field structure during SV and Cycle 1. This set of observations will produce additional flat field calibrations appropriate to the Cycle 3 time period. At one epoch during Cycle 3, high S/N spectra are obtained for G191B2B, which has a relatively featureless spectrum and which has been the primary target for earlier flat field observations. Observations are made through both the 4.3 arcsec square and the 0.25x2.0 arcsec slit aperture with all usable detector/disperser combinations. On one other occasion three REDside spectral elements will be monitored with 4.3 and slit.

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