Bibcode
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.; McMahon, R.
Referencia bibliográfica
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: 00/2002, p.117
Fecha de publicación:
1
2002
Número de citas
1
Número de citas referidas
1
Descripción
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.