Abstract / Description of output
As the epoch of spheroid formation in massive galaxies is believed to
correspond to the growth of active nuclei, probing the population of
obscured AGN at high redshift is a particularly important capability of
deep Chandra and XMM surveys. We present first results of the
ELAIS/SCUBA Chandra survey, including optical and IR spectroscopic
identifications, and explote the constraints these data place on models
of the XRB requiring a vast population of heavily obscured AGN.
Original language | English |
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Title of host publication | The High Energy Universe at Sharp Focus: Chandra Science, held in conjunction with the 113th Annual Meeting of the ASP. ASP Conference Proceedings |
Pages | 117 |
Volume | 262 |
Publication status | Published - 1 Jan 2002 |