Faint Object Spectrograph (FOS) Calibration

R. J. Harms; J. R. P. Angel; F. Bartko; E. A. Beaver; R. Bohlin; E. M. Burbidge; A. F. Davidsen; H. Ford; B. Margon; J. McCoy

doi:10.1117/12.933466

16 November 1982 Faint Object Spectrograph (FOS) Calibration

R. J. Harms, J. R. P. Angel, F. Bartko, E. A. Beaver, R. Bohlin, E. M. Burbidge, A. F. Davidsen, H. Ford, B. Margon, J. McCoy

Author Affiliations +

Proceedings Volume 0331, Instrumentation in Astronomy IV; (1982) https://doi.org/10.1117/12.933466
Event: 1982 Astronomy Conferences, 1982, Tucson, United States

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.

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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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