Galaxy population properties of the massive X-ray luminous galaxy cluster XDCP J0044.0-2033 at z = 1.58⋆⋆⋆

Author： Fassbender R.   Nastasi A.   Santos J. S.   Lidman C.   Verdugo M.   Koyama Y.   Rosati P.   Pierini D.   Padilla N.   Romeo A. D.   Menci N.   Bongiorno A.   Castellano M.   Cerulo P.   Fontana A.   Galametz A.   Grazian A.   Lamastra A.   Pentericci L.   Sommariva V.   Strazzullo V.   Šuhada R.   Tozzi P.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|568|issue|A5-A5

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.568, Iss.issue, 2014-08, pp. : A5-A5

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Abstract

Context. Recent observational progress has enabled the detection of galaxy clusters and groups out to very high redshifts and for the first time allows detailed studies of galaxy population properties in these densest environments in what was formerly known as the “redshift desert” at z> 1.5.

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