Stellar And Galactic Environment survey (SAGE)

Details Stellar And Galactic Environment survey (SAGE) Stellar And Galactic Environment survey (SAGE)

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009exa....23..169b&link_type=abstract

Experimental Astronomy, Volume 23, Issue 1, pp.169-191

Astronomy and Astrophysics

Astronomy

2

Stars, White Dwarfs, Agn, Cataclysmic Variables, Extreme Ultraviolet, Spectroscopy, Gratings, Mcp Detectors

Scientific paper

This paper describes a proposed high resolution soft X-ray and Extreme Ultraviolet spectroscopy mission to carry out a survey of Stellar and Galactic Environments (SAGE). The payload is based on novel diffraction grating technology which has already been proven in a sub-orbital space mission and which is ready to fly on a satellite platform with minimal development. We discuss the goals of a SAGE base-line mission and demonstrate the scientific importance of high resolution spectroscopy in the Extreme Ultraviolet for the study of stars and the local interstellar medium.

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