English

INTEGRAL - a status report

High Energy Astrophysical Phenomena 2010-11-02 v1 Instrumentation and Methods for Astrophysics

Abstract

The ESA gamma-ray observatory INTEGRAL, launched on 17 October 2002, continues to produce a wealth of discoveries and new results on compact high energy Galactic objects, nuclear gamma-ray line emission, diffuse line and continuum emission, cosmic background radiation, AGN, high energy transients and sky surveys. The observing programme, fully open to the scientific community at large, is built from the community's feedback to the Announcements of Opportunity, issued about once per year. The mission's technical status is healthy and INTEGRAL is continuing its scientific operations well beyond its 5-year technical design lifetime. This paper will briefly summarize the overall current status.

Keywords

Cite

@article{arxiv.0912.0077,
  title  = {INTEGRAL - a status report},
  author = {Christoph Winkler},
  journal= {arXiv preprint arXiv:0912.0077},
  year   = {2010}
}

Comments

8 pages, invited paper, Proc. of Workshop "The Extreme sky: Sampling the Universe above 10 keV", Otranto (Lecce) Italy, October 13-17, 2009 Proceedings of Science, http://pos.sissa.it, accepted

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