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The medium sensitivity survey and the X-ray selected quasar sample

Published online by Cambridge University Press:  19 July 2016

Isabella M. Gioia
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass. On leave of absence from Istituto di Radioastronomia, Bologna, Italy
Tommaso Maccacaro
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass. On leave of absence from Istituto di Radioastronomia, Bologna, Italy
Rudolph Schild
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass.
John Stocke
Affiliation:
Center for Astrophysics and Space Astronomy, Boulder, Colorado
John Danziger
Affiliation:
European Southern Observatory, Garching bei Munchen, FRG

Abstract

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We find that the inconsistencies discussed by many authors between the expected and observed number of X-ray selected quasars cannot be attributed to incompleteness of the Medium Sensitivity Survey (MSS). We are presently expanding the survey, this effort will produce a very large sample of X-ray selected quasars. Preliminary results are presented.

Type
II. Continuum Emission
Copyright
Copyright © Reidel 1986 

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