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28 July 2000 FUV grating performance for the cosmic origins spectrograph
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Abstract
The Cosmic Origins Spacecraft (COS) will be the most sensitive UV spectrograph to be flown aboard the Hubble Space Telescope. The COS FUV and NUV channels will provide high sensitivity at resolution greater than 20000 over wavelengths ranging from 115 nm to 320 nm. We present a brief review of the instrument design and grating test plan as well optical test results for the first FUV grating delivered.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Steven N. Osterman, Erik Wilkinson, James C. Green, and Kevin W. Redman "FUV grating performance for the cosmic origins spectrograph", Proc. SPIE 4013, UV, Optical, and IR Space Telescopes and Instruments, (28 July 2000); https://doi.org/10.1117/12.394019
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