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16 November 1982 Faint Object Spectrograph (FOS) Calibration
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Abstract
The Faint Object Spectrograph (FOS) designed for use with The Space Telescope (ST), is currently preparing for instrument assembly, integration, alignment, and calibration. Nearly all optical and detector elements have been completed and calibrated, and selection of flight detectors and all but a few optical elements has been made. Calibration results for the flight detectors and optics are presented, and plans for forthcoming system calibration are briefly described.
© (1982) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
R. J. Harms, J. R. P. Angel, F. Bartko, E. A. Beaver, R. Bohlin, E. M. Burbidge, A. F. Davidsen, H. Ford, B. Margon, and J. McCoy "Faint Object Spectrograph (FOS) Calibration", Proc. SPIE 0331, Instrumentation in Astronomy IV, (16 November 1982); https://doi.org/10.1117/12.933466
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