Overview of the Cosmic Origins Spectrograph Performance After the 1st Year On-Orbit

Details Overview of the Cosmic Origins Spectrograph Performance After the 1st Year On-Orbit Overview of the Cosmic Origins Spectrograph Performance After the 1st Year On-Orbit

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21725401o&link_type=abstract

American Astronomical Society, AAS Meeting #217, #254.01; Bulletin of the American Astronomical Society, Vol. 43, 2011

Computer Science

Performance

Scientific paper

The Cosmic Origins Spectrograph (COS) was installed on board the Hubble Space Telescope (HST) in May 2009 as part of the most recent servicing mission 4, and is a third-generation instrument that has significantly extended the HST UV spectroscopic capabilities. Here we highlight the current instrument performance, with particular emphasis on the calibrations performed during Cy 17. Plans for future improvements in the COS on-orbit calibration are also discussed.

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