. (2009) Stellar and galactic environment survey (SAGE). Experimental Astronomy, Vol.23 (No.1). pp. 169-191. ISSN 0922-6435

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Abstract

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.

Item Type:	Journal Article
Subjects:	Q Science > QB Astronomy
Divisions:	Faculty of Science > Physics
Library of Congress Subject Headings (LCSH):	Ultraviolet spectroscopy, Cataclysmic variable stars, White dwarf stars, Active galactic nuclei
Journal or Publication Title:	Experimental Astronomy
Publisher:	Springer
ISSN:	0922-6435
Date:	March 2009
Volume:	Vol.23
Number:	No.1
Number of Pages:	23
Page Range:	pp. 169-191
Identification Number:	10.1007/s10686-008-9105-x
Status:	Peer Reviewed
Publication Status:	Published
Access rights to Published version:	Restricted or Subscription Access
Funder:	United States. Office of Naval Research (ONR), Naval Research Laboratory (U.S.) (NRL), United States. National Aeronautics and Space Administration (NASA), Particle Physics and Astronomy Research Council (Great Britain) (PPARC), Science and Technology Facilities Council (Great Britain) (STFC)
Grant number:	W.U.3641 (ONR), 76-6039 (NRL), S-47440F (NASA), W-19,881 (NASA)
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URI:	http://wrap.warwick.ac.uk/id/eprint/28478

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