Johnson, O.; Almaini, O.; Lawrence, A.; Manners, J.; Dunlop, J.; Mann, B.; Perez Fournon, I.; Gonzales Solares, E.; Willott, C.; Oliver, S.; Rowan-Robinson, M.; Serjeant, S.; Ciliegi, P. and McMahon, R.
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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.
|Item Type:||Conference Item|
|Extra Information:||The High Energy Universe at Sharp Focus: Chandra Science, held in conjunction with the 113th Annual Meeting of the ASP. ASP Conference Proceedings, Vol. 262. Edited by Eric M. Schlegel and Saeqa Dil Vrtilek. ISBN: 1-58381-102-8. San Francisco: Astronomical Society of the Pacific, 2002. Publication Date: 2002, p.117|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Users 13 not found.|
|Date Deposited:||08 Nov 2006|
|Last Modified:||04 Oct 2016 09:56|
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