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Clustering of galaxies in the overdense regions of radio galaxies at z>0.6

Published online by Cambridge University Press:  01 August 2006

Nedelia A. Popescu
Nedelia A. Popescu*
Affiliation:
Astronomical Institute of Romanian Academy, Bucharest, RO-040557, Romania email: nedelia@aira.astro.ro
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Abstract

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Photometric redshifts technique and red sequence technique are used in order to analyze the clustering of galaxies in the environments of 4 radio galaxies with redshifts z>0.6.

Keywords

galaxies: photometrygalaxies: distances and redshiftsgalaxies: clusters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 421
Copyright
Copyright © International Astronomical Union 2007

References

Stanford, S. A., Eisenhardt, P., Dickinson, M., Holden, B., & De Propris, R. 2002, ApJS 142, 153.CrossRefGoogle Scholar
Le Borgne, D. & Rocca-Volmerange, B. 2002, A&A 386, 446.Google Scholar
Popescu, N. A. 2006, Rom.Astron.J.S. 16, 135.Google Scholar