Hostname: page-component-cc8bf7c57-5wl6q Total loading time: 0 Render date: 2024-12-12T06:46:02.111Z Has data issue: false hasContentIssue false
  • English
  • Français

The Next Generation of High-energy Astrophysics Observatories

Published online by Cambridge University Press:  25 May 2016

S. S. Holt
S. S. Holt*
Affiliation:
Goddard Space Flight Center, Code 600, Greenbelt MD 20771, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The sky will soon be populated with a fleet of new X- and gamma-ray satellites with extraordinary capabilities. This paper is meant to introduce these new missions, Chandra, XMM, and Astro-E, which will provide a large fraction of our high energy “space observatory” functionality for the next decade.

Type
Part I: Talks
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 5 - 13
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Bowyer, S., Byram, E. T., Chubb, T. A., & Friedman, H. 1964, Science, 146, 912.CrossRefGoogle Scholar
Clark, G., Garmire, G., Oda, M., Wada, M., Giacconi, R., Gursky, H., & Waters, J. R. 1965, Nature, 207, 584.CrossRefGoogle Scholar
Gold, T. 1968, Nature, 218, 731.CrossRefGoogle Scholar
Holt, S. S. 1987, Astrophys. Lett., 26, 61.Google Scholar
Perlmutter, S., et al. 1999, ApJ, 517, 565.CrossRefGoogle Scholar
Schreier, E., Levinson, R., Gursky, H., Kellogg, E., Tananbaum, H., & Giacconi, R. 1972, ApJ, 172, L79.CrossRefGoogle Scholar
Serlemitsos, P. J., Boldt, E. A., Holt, S. S., Ramaty, R., & Brisken, A. F. 1973, ApJ, 184, L1.CrossRefGoogle Scholar
White, N. E. 2000, these Proceedings.CrossRefGoogle Scholar