FUV grating performance for the cosmic origins spectrograph

Details FUV grating performance for the cosmic origins spectrograph FUV grating performance for the cosmic origins spectrograph

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spie.4013..360o&link_type=abstract

Proc. SPIE Vol. 4013, p. 360-366, UV, Optical, and IR Space Telescopes and Instruments, James B. Breckinridge; Peter Jakobsen; E

Physics

1

Scientific paper

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.

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