Unconventional AGN in hard X-ray surveys
β Scribed by A. Comastri; M. Brusa; M. Mignoli; The Hellas2xmm Team
- Publisher
- John Wiley and Sons
- Year
- 2003
- Tongue
- English
- Weight
- 187 KB
- Volume
- 324
- Category
- Article
- ISSN
- 0004-6337
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β¦ Synopsis
Abstract
Extensive programs of followβup observations of hard Xβray selected sources have unambiguously revealed that the sources of the Xβray background are characterized by an extremely large dispersion in their optical magnitude and spectroscopic classification. Here we present the results of an attempt to understand the nature of the observed variety using a simple prescription for their optical to Xβray energy distribution.
π SIMILAR VOLUMES
One of the few remaining astronomical bands (factor of -10 in energy range) still without an all-sky imaging survey is the hard x-ray band (10-600 keV). This is in spite of sensitive imaging all-sky surveys already conducted at soft x-ray (0.2-2 keV; ROSAT) and soft/hard y-ray (-750 keV -10 GeV; COM
The BeppoSAX High Energy Large Area Survey (HELLAS) has found so far 200 sources with a 5-10 flux higher than 5 Γ 10 -14 erg cm -2 s -1 in βΌ 80 deg 2 of sky. A summary on the optical identifications of a subsample of these sources is presented here. Most of the identified sources are AGN at 0.04<z<3