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Optical and Near-Infrared Photometry of Distant Galaxy Clusters

S. A. Stanford·Peter R. Eisenhardt·Mark Dickinson·B. P. Holden·Roberto De Propris
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Abstract

We present optical and near-infrared photometry of 45 clusters of galaxies at 0.1 < z < 1.3. Galaxy catalogs in each cluster were defined at the longest wavelenth available, generally the K-band, down to approximately two magnitudes below M*. We include finding chart images of the band used for catalog definition. The photometry has been used in previously published papers to examine the origin and evolution of galaxies in distant clusters.

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S. A. Stanford, Peter R. Eisenhardt, Mark Dickinson, B. P. Holden, Roberto De Propris. 2002-04-10. Optical and Near-Infrared Photometry of Distant Galaxy Clusters. https://doi.org/10.1086/340972

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