ChaMP and the High Redshift Quasars in X-rays

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dc.creatorMathur, S.
dc.creatorMarshall, H.
dc.creatorEvans, N.
dc.creatorGreen, P.
dc.creatorWilkes, B.
dc.date2000-02-01
dc.date.accessioned2026-07-07T01:52:03Z
dc.date.available2026-07-07T01:52:03Z
dc.descriptionChandra X-ray Observatory, (formerly known as AXAF), will observe down to the flux limit of 2\times 10^{-16} erg~s^{-1} cm^{-2}. In its first year of operation Chandra's CCD detectors will observe over 1500 quasars serendipitously in the soft (0.5--3.5 keV) band. Over 200 quasars will be detected in X-rays in the redshift range 3<z<4 and over 400 quasars in 2<z<3. This will enable us to determine the high redshift X-ray luminosity function. This is the contribution by unabsorbed sources only. The total numbers would be larger by about 60%
dc.descriptionTo apper in "The Hy-Redshift Universe: Galaxy Formation and Evolution at High Redshift", edited by Andrew J. Bunker & Wil J. M. van Breugel. 4 pages, LaTex, requires paspconf.sty, included
dc.identifierhttps://arxiv.org/abs/astro-ph/0002028
dc.identifierhttp://arxiv.org/abs/astro-ph/0002028
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/492
dc.subjectAstrophysics
dc.titleChaMP and the High Redshift Quasars in X-rays
dc.typetext

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