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X-ray QSO evolution from a very deep ROSAT surveySome 32 quasi-stellar objects (QSOs) were identified to a flux limit of 2 x 10(exp -15) erg/sq cm in the deepest optically identified X-ray survey performed to date. This Rosat position sensitive proportional counter survey (PSPC) is spectroscopically 86 percent complete. The surface density of quasars at this flux limit is 210 +/- 37 per sq deg. The QSO X-ray luminosity function was measured at low luminosities and high redshifts, the highest of which was 3.4.
Document ID
19970024668
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Jones, L. R.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
McHardy, I. M.
(Southampton Univ. United Kingdom)
Merrifield, M. R.
(Southampton Univ. United Kingdom)
Mason, K. O.
(University Coll. Holmbury Saint Mar, United Kingdom)
Smith, P. J.
(University Coll. Holmbury Saint Mar, United Kingdom)
Abraham, R. G.
(Institute of Astronomy Cambridge, United Kingdom)
Branduardi-Raymont, G.
(University Coll. Holmbury Saint Mar, United Kingdom)
Newsam, A. M.
(Southampton Univ. United Kingdom)
Romero-Colmanero, E.
(University Coll. Holmbury Saint Mar, United Kingdom)
Date Acquired
August 17, 2013
Publication Date
February 1, 1996
Subject Category
Space Radiation
Accession Number
97N24425
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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