The cosmic origins spectrograph: A hubble replacement instrument for the 2002 reservicing mission

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 3356, Issue , 1998, Pages 265-270

  Green, James C ^a  

^a UNIVERSITY OF COLORADO   (United States)

Author keywords

HST; Space; Spectrograph; Ultraviolet

Indexed keywords

COSMIC ORIGINS SPECTROGRAPHS; EVOLUTION OF GALAXIES; HST; HUBBLE SPACE TELESCOPES; INTERSTELLAR MEDIUMS; LARGE SCALE STRUCTURES; SPACE; ULTRAVIOLET;

ASTRONOMY; SPACE TELESCOPES; SPECTROGRAPHS; AIRBORNE TELESCOPES; OPTICAL DESIGN; OPTICAL TELESCOPES; ULTRAVIOLET RADIATION;

INSTRUMENTS; INFRARED SPECTROGRAPHS;

COSMIC ORIGINS SPECTROGRAPHS (COS); HUBBLE SPACE TELESCOPES (HST);

EID: 0032299078     PISSN: 0277786X     EISSN: 1996756X     Source Type: Conference Proceeding    
DOI: 10.1117/12.324466     Document Type: Conference Paper

References (3)

1. J. Sanhow, S. D. Friedman, W. R. Oegerle, H. W. Moos, J. C. Green, and 0. H. W. Siegmund, "Design and Predicted Performance of the Far Ultraviolet Spectroscopic Explorer (FUSE),' SPIE, vol. 2807,pp. 2-101996.
2. H. W. Siegmund, et al, "Performance of the Double Delay Line Microchannel Plate Detectors for the Far Ultraviolet Spectroscopic Explorer," SPIE, vol. 3114, pp. 283-294, 1997.
3. Madau and A. Meiksin, "The He II Lyman-Alpha Opacity of the Universe," Astrophysical Journal (letters), vol. 433, pp. L53-L56