The Cosmic Origins Spectrograph (COS): high-senitivity UV spectroscopy with HST.

Details The Cosmic Origins Spectrograph (COS): high-senitivity UV spectroscopy with HST. The Cosmic Origins Spectrograph (COS): high-senitivity UV spectroscopy with HST.

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998stsin..15....6g&link_type=abstract

Space Telesc. Sci. Inst., Newsl., Vol. 15, No. 1, p. 6 - 7, 21

Physics

Hubble Space Telescope: Uv Spectrographs

Scientific paper

The Cosmic Origins Spectrograph (COS) has been selected as a replacement instrument for the fourth HST servicing mission in 2002. COS is a high-throughput ultraviolet spectrograph that is optimized to observe faint point sources. Two gratings are used to cover the 1150 Å to 1775 Å region at high resolution (R = 20,000 to 24,000). A third grating covers the entire 1230 Å to 2050 Å region at lower resolution (R = 2500 to 3500).

Affiliated with

Also associated with

No associations

Rating

The Cosmic Origins Spectrograph (COS): high-senitivity UV spectroscopy with HST. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Cosmic Origins Spectrograph (COS): high-senitivity UV spectroscopy with HST., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Cosmic Origins Spectrograph (COS): high-senitivity UV spectroscopy with HST. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1615670