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Spatial Correlation Functions of Bright Radio Galaxies

Published online by Cambridge University Press:  03 August 2017

You-yuan Zhou  and
Yi-peng Jing
You-yuan Zhou
Affiliation:
Center for Astrophysics, University of Science and Technology of China, Hefei. Anhui, China
Yi-peng Jing
Affiliation:
Center for Astrophysics, University of Science and Technology of China, Hefei. Anhui, China

Extract

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Because of their large separation bright radio galaxies characterize the structure of the universe on the scales of clusters and superclusters. In order to calculate the spatial correlation function we choose radio galaxies in radio surveys, for which the redshift values have been measured. One is from Bright Radio Sources at 178 MHz (Liang, Riley and Longair 1983), and another is from All-Sky Catalogue of Bright Extragalactic Radio Sources at 2.7 GHz (Wall and Peacock 1985).

Type
Appendix 1: Poster Papers
Information
Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 580
Copyright
Copyright © Reidel 1988