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 suborbital 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.
Stellar and galactic environment survey (SAGE) / 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., Kappelmann, N., et al.. - In: ASTROPHYSICS AND SPACE SCIENCE. - ISSN 0004-640X. - STAMPA. - 320:(2009), pp. 231-238. [10.1007/s10509-008-9792-9]
Stellar and galactic environment survey (SAGE)
PACE, EMANUELE;
2009
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 suborbital 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.| File | Dimensione | Formato | |
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