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- W2160779387 abstract "Galaxy clusters at are particularly important in the study of cluster evolution and the application of clusters to cosmological studies. We briefly discuss the difficulties in creating well-defined, large, high-redshift cluster samples, and some of the techniques used in optical/IR imaging to overcome them. We give a summary of the current state of optical/IR observations of the relatively small number of high-redshift clusters identified so far, including discussions of the galaxy luminosity function, the Fundamental Plane, the color-magnitude relation, and the Butcher-Oemler effect. The application of photometric redshift techniques is also highlighted.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html" @default.
- W2160779387 created "2016-06-24" @default.
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- W2160779387 date "2004-03-01" @default.
- W2160779387 modified "2023-09-25" @default.
- W2160779387 title "Optical/infrared observations of high-redshift galaxy clusters" @default.
- W2160779387 doi "https://doi.org/10.1017/s1743921304000389" @default.
- W2160779387 hasPublicationYear "2004" @default.
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