The INTEGRAL mission an overview
Abstract
The ESA observatory INTEGRAL (International Gamma-Ray Astrophysics Laboratory) is dedicated to fine imaging and spectroscopy in the energy range 15 keV to 10 Mev with concurrent X-ray (3-35 keV) and optical monitoring. It was launched on October 17, 2002 and has been succesfully operating ever since. Its two main instruments the spectrometer SPI - optimized for high resolution spectroscopy - and the imager IBIS - optimized for for high resolution imaging - are complemented by the X-ray monitor JEM-X and the optical monitor OMC. All the high energy instruments use coded mask techniques, allowing imaging in the gamma-ray range and combining wide fields of view with high spatial resolution. The presentation gives an overview of the unique properties of INTEGRAL.
- Publication:
-
Populations of High Energy Sources in Galaxies
- Pub Date:
- 2006
- DOI:
- 10.1017/S1743921306007873
- Bibcode:
- 2006IAUS..230...59K