Stellar mass-halo mass relation for the brightest central galaxies of X-ray clusters since z ∼ 0.65
- G. Erfanianfar*
- , A. Finoguenov
- , K. Furnell
- , P. Popesso
- , A. Biviano
- , S. Wuyts
- , C. A. Collins
- , M. Mirkazemi
- , J. Comparat
- , H. Khosroshahi
- , K. Nandra
- , R. Capasso
- , E. Rykoff
- , D. Wilman
- , A. Merloni
- , N. Clerc
- , M. Salvato
- , J. I. Chitham
- , L. S. Kelvin
- , G. Gozaliasl
*Corresponding author for this work
- Max Planck Institute for Extraterrestrial Physics
- University of Helsinki
- Liverpool John Moores University
- Excellence Cluster Universe
- Osservatorio Astronomico di Trieste
- University of Bath
- Institute for Research in Fundamental Sciences
- Ludwig Maximilian University of Munich
- Stanford University
- SLAC National Accelerator Laboratory
- Université Paul Sabatier Toulouse III
- University of Turku
- University of St Andrews
- University of Utah
- University of Arizona
- Pennsylvania State University
Research output: Contribution to journal › Article › Scientific › peer-review
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