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Variation of Radio Source Counts with Direction, for the 3CR and 4C Surveys

Pearson, T. J. (1974) Variation of Radio Source Counts with Direction, for the 3CR and 4C Surveys. Monthly Notices of the Royal Astronomical Society, 166 (2). pp. 249-258. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20200608-115353608

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Abstract

In an investigation of variations with direction of the radio source counts N(S) for the 3CR and 4C surveys, no anisotropy has been found which is not explicable in terms of random statistical differences between limited samples of sources; in particular, there is no significant difference between the slopes of the source counts in the northern and southern galactic hemispheres.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/166.2.249DOIArticle
https://ui.adsabs.harvard.edu/abs/1974MNRAS.166..249P/abstractADSArticle
ORCID:
AuthorORCID
Pearson, T. J.0000-0001-5213-6231
Additional Information:© 1974 Royal Astronomical Society. Provided by the NASA Astrophysics Data System. (Received 1973 September 19) I thank Dr M. S. Longair and the other members of the Mullard Radio Astronomy Observatory who have given me advice and criticism, and I am indebted to the Science Research Council for a Research Studentship.
Funders:
Funding AgencyGrant Number
Science Research Council (SRC)UNSPECIFIED
Issue or Number:2
Record Number:CaltechAUTHORS:20200608-115353608
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200608-115353608
Official Citation:T. J. Pearson, Variation of Radio Source Counts with Direction, for the 3CR and 4C Surveys, Monthly Notices of the Royal Astronomical Society, Volume 166, Issue 2, February 1974, Pages 249–258, https://doi.org/10.1093/mnras/166.2.249
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:103759
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:08 Jun 2020 22:44
Last Modified:08 Jun 2020 22:44

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