Abstract
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 |