Stellar and galactic environment survey (SAGE)

M. A. Barstow; M. R. Burleigh; N. J. Bannister; J. S. Lapington; M. P. Kowalski; R. G. Cruddace; K. S. Wood; F. Auchere; M. F. Bode; G. E. Bromage; B. Gibson; Andrew Collier Cameron; A. Cassatella; F. Delmotte; M.-F. Ravet; J. G. Doyle; C. S. Jeffery; B. Gaensicke; C. Jordan; N. Kappelmann; K. Werner; R. Lallement; D. de Martino; S. A. Matthews; K. J. H. Phillips; G. Del Zanna; M. Orio; E. Pace; I. Pagano; J. H. M. M. Schmitt; B. Y. Welsh

doi:10.1007/s10509-008-9792-9

Stellar and galactic environment survey (SAGE)

M. A. Barstow, M. R. Burleigh, N. J. Bannister, J. S. Lapington, M. P. Kowalski, R. G. Cruddace, K. S. Wood, F. Auchere, M. F. Bode, G. E. Bromage, B. Gibson, Andrew Collier Cameron, A. Cassatella, F. Delmotte, M.-F. Ravet, J. G. Doyle, C. S. Jeffery, B. Gaensicke, C. Jordan, N. KappelmannK. Werner, R. Lallement, D. de Martino, S. A. Matthews, K. J. H. Phillips, G. Del Zanna, M. Orio, E. Pace, I. Pagano, J. H. M. M. Schmitt, B. Y. Welsh

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

This paper describes a proposed high resolution soft X-ray and Extreme Ultraviolet (EUV) 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. Much of the technical detail of the instrumentation has been reported elsewhere and we concentrate our discussion here on the scientific goals of a SAGE base-line mission, demonstrating the scientific importance of high resolution spectroscopy in the Extreme Ultraviolet for the study of stars and the local interstellar medium.

Original language	English
Pages (from-to)	231-238
Journal	Astrophysics and Space Science
Volume	320
Issue number	1-3
DOIs	https://doi.org/10.1007/s10509-008-9792-9
Publication status	Published - Apr 2009

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10.1007/s10509-008-9792-9

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Barstow, M. A., Burleigh, M. R., Bannister, N. J., Lapington, J. S., Kowalski, M. P., Cruddace, R. G., Wood, K. S., Auchere, F., Bode, M. F., Bromage, G. E., Gibson, B., Cameron, A. C., Cassatella, A., Delmotte, F., Ravet, M.-F., Doyle, J. G., Jeffery, C. S., Gaensicke, B., Jordan, C., ... Welsh, B. Y. (2009). Stellar and galactic environment survey (SAGE). Astrophysics and Space Science, 320(1-3), 231-238. https://doi.org/10.1007/s10509-008-9792-9

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title = "Stellar and galactic environment survey (SAGE)",

abstract = "This paper describes a proposed high resolution soft X-ray and Extreme Ultraviolet (EUV) 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. Much of the technical detail of the instrumentation has been reported elsewhere and we concentrate our discussion here on the scientific goals of a SAGE base-line mission, demonstrating the scientific importance of high resolution spectroscopy in the Extreme Ultraviolet for the study of stars and the local interstellar medium.",

author = "Barstow, {M. A.} and Burleigh, {M. R.} and Bannister, {N. J.} and Lapington, {J. S.} and Kowalski, {M. P.} and Cruddace, {R. G.} and Wood, {K. S.} and F. Auchere and Bode, {M. F.} and Bromage, {G. E.} and B. Gibson and Cameron, {Andrew Collier} and A. Cassatella and F. Delmotte and M.-F. Ravet and Doyle, {J. G.} and Jeffery, {C. S.} and B. Gaensicke and C. Jordan and N. Kappelmann and K. Werner and R. Lallement and {de Martino}, D. and Matthews, {S. A.} and Phillips, {K. J. H.} and {Del Zanna}, G. and M. Orio and E. Pace and I. Pagano and Schmitt, {J. H. M. M.} and Welsh, {B. Y.}",

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doi = "10.1007/s10509-008-9792-9",

language = "English",

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Barstow, MA, Burleigh, MR, Bannister, NJ, Lapington, JS, Kowalski, MP, Cruddace, RG, Wood, KS, Auchere, F, Bode, MF, Bromage, GE, Gibson, B, Cameron, AC, Cassatella, A, Delmotte, F, Ravet, M-F, Doyle, JG, Jeffery, CS, Gaensicke, B, Jordan, C, Kappelmann, N, Werner, K, Lallement, R, de Martino, D, Matthews, SA, Phillips, KJH, Del Zanna, G, Orio, M, Pace, E, Pagano, I, Schmitt, JHMM & Welsh, BY 2009, 'Stellar and galactic environment survey (SAGE)', Astrophysics and Space Science, vol. 320, no. 1-3, pp. 231-238. https://doi.org/10.1007/s10509-008-9792-9

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AU - Barstow, M. A.

AU - Burleigh, M. R.

AU - Bannister, N. J.

AU - Lapington, J. S.

AU - Kowalski, M. P.

AU - Cruddace, R. G.

AU - Wood, K. S.

AU - Auchere, F.

AU - Bode, M. F.

AU - Bromage, G. E.

AU - Gibson, B.

AU - Cameron, Andrew Collier

AU - Cassatella, A.

AU - Delmotte, F.

AU - Ravet, M.-F.

AU - Doyle, J. G.

AU - Jeffery, C. S.

AU - Gaensicke, B.

AU - Jordan, C.

AU - Kappelmann, N.

AU - Werner, K.

AU - Lallement, R.

AU - de Martino, D.

AU - Matthews, S. A.

AU - Phillips, K. J. H.

AU - Del Zanna, G.

AU - Orio, M.

AU - Pace, E.

AU - Pagano, I.

AU - Schmitt, J. H. M. M.

AU - Welsh, B. Y.

PY - 2009/4

Y1 - 2009/4

N2 - This paper describes a proposed high resolution soft X-ray and Extreme Ultraviolet (EUV) 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. Much of the technical detail of the instrumentation has been reported elsewhere and we concentrate our discussion here on the scientific goals of a SAGE base-line mission, demonstrating the scientific importance of high resolution spectroscopy in the Extreme Ultraviolet for the study of stars and the local interstellar medium.

AB - This paper describes a proposed high resolution soft X-ray and Extreme Ultraviolet (EUV) 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. Much of the technical detail of the instrumentation has been reported elsewhere and we concentrate our discussion here on the scientific goals of a SAGE base-line mission, demonstrating 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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DO - 10.1007/s10509-008-9792-9

M3 - Article

SN - 0004-640X

VL - 320

SP - 231

EP - 238

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

IS - 1-3

ER -

Stellar and galactic environment survey (SAGE)

Abstract

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Astrophysics in St Andrews: Astrophysics in St Andrews / SUPA (Continuan of Rolling Grant - XPP089

Wide Area Search for Planets: Project support for the Wide Area Search for Planets

Astrophysics at St Andrews: Astrophysics at St.Andrews

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Stellar and galactic environment survey (SAGE)

Abstract

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Projects

Astrophysics in St Andrews: Astrophysics in St Andrews / SUPA (Continuan of Rolling Grant - XPP089

Wide Area Search for Planets: Project support for the Wide Area Search for Planets

Astrophysics at St Andrews: Astrophysics at St.Andrews

Cite this