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Faint Object Spectrograph (FOS) calibrationThe 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.
Document ID
19830050793
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Harms, R. J. (California Univ. La Jolla, CA, United States)
Beaver, E. A. (California Univ. La Jolla, CA, United States)
Burbidge, E. M. (California, University La Jolla, CA, United States)
Angel, J. R. P. (Steward Observatory Tucson, AZ, United States)
Bartko, F. (California Univ. La Jolla, CA, United States)
Mccoy, J. (California Univ. La Jolla, CA, United States)
Ripp, L. (Martin Marietta Aerospace Denver, CO, United States)
Bohlin, R. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Davidsen, A. F. (Johns Hopkins University Baltimore, MD, United States)
Ford, H. (California, University Los Angeles, CA, United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1982
Subject Category
Instrumentation And Photography
Meeting Information
Meeting: Instrumentation in astronomy IV; Fourth Conference
Location: Tucson, AZ
Start Date: March 8, 1982
End Date: March 10, 1982
Accession Number
83A32011
Funding Number(s)
CONTRACT_GRANT: NAS5-24463
Distribution Limits
Public
Copyright
Other

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