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The Clustering and Evolution of Optically-Selected QSOs

Published online by Cambridge University Press:  19 July 2016

B.J. Boyle ,
T. Shanks ,
R. Fong  and
B.A. Peterson
B.J. Boyle
Affiliation:
University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, U.K.
T. Shanks
Affiliation:
University of Durham, South Road, Durham DH1 3LE, U.K.
R. Fong
Affiliation:
University of Durham, South Road, Durham DH1 3LE, U.K.
B.A. Peterson
Affiliation:
Mount Stromlo and Siding Spring Observatories Woden, ACT 2606, Australia

Abstract

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We are in the process of compiling a large catalogue of faint (B < 20.9 mag), UVX selected QSOs with complete spectroscopic identification using the fibre optic (FOCAP) system at the Anglo-Australian Telescope. From the 220 QSOs thus far identified we find that QSO evolution is most simply parameterised by a uniform increase in luminosity towards higher redshifts. We also find evidence for strong QSO clustering at scales < 10h−1 Mpc.

Type
Chapter XI: Quasi-Stellar Objects: Distribution and General Properties
Information
Symposium - International Astronomical Union , Volume 124: Observational Cosmology , 1987 , pp. 643 - 647
Copyright
Copyright © Reidel 1987 

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