We study the evolution of two fundamental properties of galaxy clusters: the luminosity function (LF) and the scaling relations between the total galaxy number N (or luminosity) and the cluster mass M. Using a sample of 27 clusters (0
CITATION STYLE
Lin, Y.-T., Mohr, J. J., Gonzalez, A. H., & Stanford, S. A. (2006). Evolution of the K -Band Galaxy Cluster Luminosity Function and Scaling Relations. The Astrophysical Journal, 650(2), L99–L102. https://doi.org/10.1086/508940
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