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A uniformly selected catalogue of distant galaxy clusters

Couch, Warrick J. and Ellis, Richard S. and Malin, David F. and MacLaren, Iain (1991) A uniformly selected catalogue of distant galaxy clusters. Monthly Notices of the Royal Astronomical Society, 249 (4). pp. 606-628. ISSN 0035-8711. doi:10.1093/mnras/249.4.606. https://resolver.caltech.edu/CaltechAUTHORS:20210130-165032677

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Abstract

We present a new catalogue of faint southern galaxy clusters identified from examination of high-contrast film derivatives of a set of 55 prime focus AAT photographic plates taken in one or both of two pass-bands (J≡bⱼand F≡rF).⁠. Visual scans of these films have been compared with machine measurements of the original plates and the results demonstrate that the films offer ready access to the positions (but not photometry) of large numbers of faint objects to limiting magnitudes of bⱼ≃24.4±0.3 and rF≃22.9±0.2. Our cluster candidates are chosen according to their contrast, σc₁, above the fluctuations in the field counts as determined locally on the same film. A total of 112 candidate clusters are tabulated down to a contrast level of σc₁ = 2.0 (at which point marginal effects become apparent). Cross-correlations with published catalogues (and spectroscopic measurements) confirm that the bulk of these clusters are more distant than those found by Abell and co-workers. By applying our search criteria to simulated fields containing clusters of known richnesses, and with fluctuations in the field counts matching those seen in the data, we determine our cluster list should be complete above a limit σc₁ = 3.25. Given recent estimates of the volume density of clusters of various richnesses, our simulations predict the observed number of F clusters seen above the σc₁ = 3.25 limit, but predict too few J clusters. To test for the origin of this excess of blue clusters we have measured redshifts for 95 faint galaxies in 29 of the 44 clusters with σc₁>4.0 using a variety of telescopes and instruments. A spectroscopically complete subsample in 16 fields allows us to determine the absolute space density. The spectroscopy confirms the reality of the clusters with σc₁>4.0 and shows a redshift range for the F sample similar to that expected without luminosity or cluster evolution; the J sample extends to higher redshifts than expected. A detailed study of the highest redshift clusters suggests the abundance of high-redshift J clusters arises either from projections from foreground spiral-rich groups or via recent star formation within the distant cluster environments. In support of the latter hypothesis, we demonstrate how bursts of star formation in a subset of cluster galaxies would transform the J contrast leaving the F contrast largely unaffected – in agreement with the basic trend observed. We discuss the implications of our results for further searches for high-z clusters. Only with the advent of wide-field infrared imaging, or X-ray selected samples, might galaxy-dependent selection effects associated with variations in stellar populations at a given epoch be overcome.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/249.4.606DOIArticle
https://ui.adsabs.harvard.edu/abs/1991MNRAS.249..606C/abstractADSArticle
ORCID:
AuthorORCID
Ellis, Richard S.0000-0001-7782-7071
Additional Information:© 1991 Royal Astronomical Society. Provided by the NASA Astrophysics Data System. Accepted 1990 November 5. Received 1990 October 22; in original form 1990 August 13. This project owes much to the dedication of the staff at the Anglo-Australian Telescope, particularly its former Director, Don Morton, who encouraged the formation and exploitation of the photographic archive on which this cluster sample is based. We also thank the APM and COSMOS teams, particularly Ed Kibblewhite and Harvey MacGillivray, for their eagerness to rationalize the question of the applicability of HCFs for faint object astronomy. For the spectroscopy we thank Ian Parry and Gordon Robertson for the basis of the extraction software used, and David Allen, Jeremy Allington-Smith, Keith Taylor and Sandro D'Odorlco for their generous assistance with the various instruments used. Finally, we acknowledge encouragement from Jim Gunn and John Hoessel and useful discussions with John Lucey, Ray Sharples and Carlos Frenk.
Issue or Number:4
DOI:10.1093/mnras/249.4.606
Record Number:CaltechAUTHORS:20210130-165032677
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210130-165032677
Official Citation:Warrick J. Couch, Richard S. Ellis, David F. Malin, Iain MacLaren, A uniformly selected catalogue of distant galaxy clusters, Monthly Notices of the Royal Astronomical Society, Volume 249, Issue 4, April 1991, Pages 606–628, https://doi.org/10.1093/mnras/249.4.606
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:107829
Collection:CaltechAUTHORS
Deposited By: Rebecca Minjarez
Deposited On:05 Feb 2021 23:31
Last Modified:16 Nov 2021 19:06

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