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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
  • A. Weijmans, J. Brownstein, E. Egami, M. J. Pereira, D. P. Schneider, C. Kirkpatrick, S. Damsted, A. Kukkola
*Corresponding author for this work

Research output: Contribution to journalArticleScientificpeer-review

31 Citations (Scopus)

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