Performance of the space telescope imaging spectrograph

Details Performance of the space telescope imaging spectrograph Performance of the space telescope imaging spectrograph

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..408..483b&link_type=abstract

The ultraviolet universe at low and high redshift. AIP Conference Proceedings, Volume 408, pp. 483-492 (1997).

Computer Science

Performance

3

Space-Based Ultraviolet, Optical, And Infrared Telescopes

Scientific paper

The Space Telescope Imaging Spectrograph (STIS) was installed aboard the Hubble Space Telescope (HST) in February, 1997. STIS operates from the ultraviolet to the near infrared (115-1000 nm) in a variety of spectroscopic and imaging modes. Orbital characterization of STIS performance is currently underway and some of the initial results are presented here.

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