FOS Spectral Flat Fields Monitor, Revised

Details FOS Spectral Flat Fields Monitor, Revised FOS Spectral Flat Fields Monitor, Revised

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.4123h&link_type=abstract

HST Proposal ID #4123

Physics

Hst Proposal Id #4123

Scientific paper

In this test we will obtain spectra of standard stars with relatively
smooth continua, on a regular basis, to track the time-dependence of
flat-field structure of the FOS Red detector in the UV. Spectra will be
obtained in both the 4.3 aperture and the slit, since the flat- field
structure is dependent on aperture size.

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