Stellar mass–halo mass relation for the brightest central galaxies of X-ray clusters since z ∼ 0.65

G. Erfanianfar (1) , A. Finoguenov (1, 2) , K. Furnell (3) , P. Popesso (4) , A. Biviano (5) , S. Wuyts (6) , C. Collins (3) , M. Mirkazemi (4) , J. Comparat (1) , H. Khosroshahi (7) , K. Nandra (8) , R. Capasso (4, 9) , E. Rykoff (10, 11) , D. Wilman (8) , A. Merloni (1) , N. Clerc (12) , M. Salvato (1) , J. Chitham (1) , L. Kelvin (3) , G. Gozaliasl (13) , A. Weijmans (14) , J. Brownstein (15) , E. Egami (16) , M. Pereira (16) , D. Schneider (17) , C. Kirkpatrick (2) , S. Damsted (2) , A. Kukkola (2)

1 MPE - Max Planck Institute for Extraterrestrial Physics
2 Department of Physics [Helsinki]
3 ARI - Astrophysics Research Institute [Liverpool]
4 Excellence Cluster Universe
5 OAT - INAF - Osservatorio Astronomico di Trieste
6 University of Bath [Bath]
7 School of Astronomy and Astrophysics [Teheran]
8 MPE - Max-Planck-Institut für Extraterrestrische Physik
9 LMU - Ludwig Maximilian University [Munich] = Ludwig Maximilians Universität München
10 KIPAC - Kavli Institute for Particle Astrophysics and Cosmology
11 SLAC - SLAC National Accelerator Laboratory
12 IRAP - Institut de recherche en astrophysique et planétologie
13 Helsingin yliopisto = Helsingfors universitet = University of Helsinki
14 University of St Andrews [Scotland]
15 University of Utah
16 Steward Observatory
17 Penn State - Pennsylvania State University

Domaines: Astrophysique [astro-ph]; Astrophysique galactique [astro-ph.GA]

G. Erfanianfar, A. Finoguenov, K. Furnell, P. Popesso, A. Biviano, et al.. Stellar mass–halo mass relation for the brightest central galaxies of X-ray clusters since z ∼ 0.65. Astronomy and Astrophysics - A&A, 2019, 631, pp.A175. ⟨10.1051/0004-6361/201935375⟩. ⟨hal-02514921⟩