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arXiv 0902.4319astro-ph.GAastro-ph.HE
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Extragalactic Hard X-ray Surveys: From INTEGRAL to Simbol-X

S. Paltani, T. Dwelly, R. Walter, A. P. Marscher, S. G. Jorstad, I. M. McHardy, T. J. -L. Courvoisier

英文摘要:

We present some results of the deepest extragalactic survey performed by the INTEGRAL satellite. The fraction of very absorbed AGN is quite large. The sharp decrease in the absorption fraction with X-ray luminosity observed at lower-energy X-rays is not observed. The current lack of truly Compton-thick objects, with an upper limit of 14% to the size of this population, is just compatible with recent modeling of the cosmic X-ray background. We also study the prospects for a future hard X-ray serendipitous survey with Simbol-X. We show that Simbol-X will easily detect a large number of serendipitous AGN, allowing us to study the evolution of AGN up to redshifts about 2, opening the door to the cosmological study of hard X-ray selected AGN, which is barely possible with existing satellites like Swift and INTEGRAL.

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