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The APM galaxy survey .5. Catalogues of galaxy clusters

Abstract:
We describe the construction of catalogues of galaxy clusters from the APM Galaxy survey using an automated algorithm based on Abell-like selection criteria. We investigate the effects of varying several parameters in our selection algorithm, including the magnitude range and radius from the cluster centre used to estimate the cluster richnesses. We quantify the accuracy of the photometric distance estimates by comparing them with measured redshifts, and we investigate the stability and completeness of the resulting catalogues. We find that the angular correlation functions for different cluster catalogues are in good agreement with one another, and are also consistent with the observed amplitude of the spatial correlation function of rich clusters. © 1997 RAS.
Publication status:
Published

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Publisher copy:
10.1093/mnras/289.2.263

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author


Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
289
Issue:
2
Pages:
263-284
Publication date:
1997-08-01
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Keywords:
Pubs id:
pubs:11650
UUID:
uuid:0edaecb3-0b9e-4580-bdf9-7b6a15d8aa00
Local pid:
pubs:11650
Source identifiers:
11650
Deposit date:
2012-12-19
ARK identifier:

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