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Space Distribution of Ouasars Based on Optically Selected Samples

Published online by Cambridge University Press:  14 August 2015

Maarten Schmidt
Affiliation:
Palomar Observatory, California Institute of Technology
Richard F. Green
Affiliation:
Steward Observatory, University of Arizona

Extract

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Even though the number of known quasars is approaching 2000, relatively few belong to well defined complete samples which are needed to derive their space distribution. For many years, the Braccesi survey (Braccesi, Formiggini, and Gandolfi 1970) was the only published one — its limited spectroscopic coverage allowed construction of only a small complete sample of 19 quasars brighter than B = 18, over an area of 36 sq. deg.

Type
Research Article
Copyright
Copyright © Reidel 1982 

References

Braccesi, A., Formiggini, L., and Gandolfi, E.: 1970, Astron. Astrophys. 5, pp. 264279.Google Scholar
Kron, R. G., and Chiu, L. G.: 1981, preprint.Google Scholar
Osmer, P. S.: 1980, Astrophys. J. Suppl., 42, pp. 523540.Google Scholar
Osmer, P. S.: 1981, preprint.Google Scholar
Osmer, P. S., and Smith, M. G.: 1980, Astrophys. J. Suppl., 42, pp. 333349.Google Scholar
Ostriker, J. P., and Cowie, L. L.: 1981, Astrophys. J. (Letters) 243, pp. L127131.Google Scholar