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Stellar And Galactic Environment survey (SAGE)

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

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

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.
Original languageEnglish
Pages (from-to)169-191
JournalExperimental Astronomy
Volume23
Issue number1
DOIs
Publication statusPublished - Mar 2009

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