FOS Cycle 3 Scattered-Light Calibration

Details FOS Cycle 3 Scattered-Light Calibration FOS Cycle 3 Scattered-Light Calibration

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.5200k&link_type=abstract

HST Proposal ID #5200

Computer Science

Hst Proposal Id #5200

Scientific paper

Several late-type stars will be observed with the FOS UV gratings. The FOS observations will be compared with HRS Side 1 observations of the same stars made during Cycle 1 and SV. Since HRS Side 1 is insensitive to wavelengths longward of approximately 2000 A., any additional light detected in the FOS observations is attributable to longer-wavelength continuum light scattered off the FOS gratings; the so-called FOS Red Leak.

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