Intracluster light in clusters of galaxies at redshifts 0.4<z<0.8

L. Guennou,C. Adami,C. Da Rocha, F. Durret,Melville P. Ulmer,S. Allam,Stéphane Basa,C. Benoist,Andrea Biviano,D. Clowe, R. Gavazzi,C. Halliday,O. Ilbert,David Johnston, D. W. Just,Richard G. Kron,Jeffrey M. Kubo, V. LeBrun,P. J. Marshall,Alain Mazure, K. J. Murphy,D. N. E. Pereira,C. R. Rabaça, F. Rostagni,G. Rudnick,D. Russeil,Tim Schrabback, E. Slezak,Douglas L. Tucker,Dennis Zaritsky

arXiv: Cosmology and Nongalactic Astrophysics（2011）

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摘要

The study of intracluster light can help us to understand the mechanisms taking place in galaxy clusters, and to place constraints on the cluster formation history and physical properties. However, owing to the intrinsic faintness of ICL emission, most searches and detailed studies of ICL have been limited to redshifts z<0.4.We search for ICL in a subsample of ten clusters detected by the ESO Distant Cluster Survey (EDisCS), at redshifts 0.4更多

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