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The Angular Diameter-Redshift Test for Large Redshift Quasars

Published online by Cambridge University Press:  14 August 2015

J. M. Riley ,
M. S. Longair  and
A. Hooley
J. M. Riley
Affiliation:
Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, England.
M. S. Longair
Affiliation:
Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, England.
A. Hooley
Affiliation:
Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, England.

Abstract

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Complete samples of quasars in the 3CR and 4C catalogues have been observed with a resolution of 2″ arc in RA and 2″ cosecδ in dec with the Cambridge 5-km telescope at 5 GHz (Riley & Pooley 1975; Jenkins et al 1977), from which it has been possible to determine the overall angular sizes of their radio structures (LAS). The angular diameter-redshift test for quasars has been reexamined using these data; details are described fully elsewhere (Hooley et al 1977).

Type
III. Angular Diameter-Redshift and Flux Density Tests
Information
Symposium - International Astronomical Union , Volume 74: Radio Astronomy and Cosmology , 1977 , pp. 133 - 138
Copyright
Copyright © Reidel 1977 

References

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