Resolving the hydrostatic mass profiles of galaxy clusters at z ∼ 1 with XMM-Newton and Chandra

Author: Bartalucci I.   Arnaud M.   Pratt G.W.   Le Brun A. M. C.  

Publisher: Edp Sciences

E-ISSN: 1432-0746|617|issue|A64-A64

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.617, Iss.issue, 2018-09, pp. : A64-A64

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Abstract