The extra-galactic hard x-ray sky as painted by INTEGRAL
The extra-galactic hard x-ray sky as painted by INTEGRAL
The INTEGRAL/IBIS is surveying a large fraction of the sky above 20 keV with a sensitivity larger than a few mCrab, discovering a number of new extragalactic sources many of which now identified as nearby AGN. We have combined INTEGRAL data with 2–10 keV information (XMM-Newton, Chandra, Swift, archival ASCA and BeppoSAX data) to probe the broad-band spectral properties of different classes of AGN: type 1/2 Seyfert galaxies, radio-galaxies, NLSyls, quasars. A number of interesting sources have also been discovered by means of multiwavelength observations. A study of a complete (20–40 keV) sample of AGN is on-going focused on a detailed study of the intrinsic and reflected continuum components.
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Panessa, F.
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De Rosa, A.
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Bassani, L.
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Bird, A.
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Dean, A.
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Malizia, A.
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Masetti, N.
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Molina, M.
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Ubertini, P.
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11 May 2009
Panessa, F.
ea57d0af-2ad5-4f65-a8f7-b001e70ebe13
De Rosa, A.
b2a68e71-5c23-4649-94f0-1d8ffd40bb77
Bassani, L.
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Bird, A.
045ee141-4720-46fd-a412-5aa848a91b32
Dean, A.
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Malizia, A.
efa63850-cf26-482c-ae3b-54b0c8fb8a87
Masetti, N.
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Molina, M.
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Ubertini, P.
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Panessa, F., De Rosa, A., Bassani, L., Bird, A., Dean, A., Malizia, A., Masetti, N., Molina, M. and Ubertini, P.
(2009)
The extra-galactic hard x-ray sky as painted by INTEGRAL.
Simbol-X: focusing on the hard x-ray universe: Proceedings of the 2nd International Simbol-X Symposium.
.
(doi:10.1063/1.3149390).
Record type:
Conference or Workshop Item
(Paper)
Abstract
The INTEGRAL/IBIS is surveying a large fraction of the sky above 20 keV with a sensitivity larger than a few mCrab, discovering a number of new extragalactic sources many of which now identified as nearby AGN. We have combined INTEGRAL data with 2–10 keV information (XMM-Newton, Chandra, Swift, archival ASCA and BeppoSAX data) to probe the broad-band spectral properties of different classes of AGN: type 1/2 Seyfert galaxies, radio-galaxies, NLSyls, quasars. A number of interesting sources have also been discovered by means of multiwavelength observations. A study of a complete (20–40 keV) sample of AGN is on-going focused on a detailed study of the intrinsic and reflected continuum components.
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Published date: 11 May 2009
Venue - Dates:
Simbol-X: focusing on the hard x-ray universe: Proceedings of the 2nd International Simbol-X Symposium, 2009-05-11
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Local EPrints ID: 144783
URI: http://eprints.soton.ac.uk/id/eprint/144783
PURE UUID: 7d95ce22-fd3d-4a6a-9a6d-a78ae7526545
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Date deposited: 25 May 2010 10:59
Last modified: 14 Mar 2024 02:36
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Contributors
Author:
F. Panessa
Author:
A. De Rosa
Author:
L. Bassani
Author:
A. Dean
Author:
A. Malizia
Author:
N. Masetti
Author:
M. Molina
Author:
P. Ubertini
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