FOS Instrument Science Report 115

"Scattered Light in the G130H and G190H Modes of the HST Faint Object 
Spectograph"
by T.R. Ayres

Abstract excerpted from the report:
	Grating scattered light can be a significant problem for FOS
	spectroscopy of "red" celestial objects below 2000A. It can be 
	quantified empirically through comparisons of G130H and G190H
	spectraof solar-type stars with templates based on irradiance scans of
	the Sun and IUE exposures of field G-type dwarfs.





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