Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z <1.3

Ghassem Gozaliasl, Alexis Finoguenov, Habib G. Khosroshahi, Bruno M. B. Henriques, Masayuki Tanaka, Olivier Ilbert, Stijn Wuyts, Henry J. McCracken, Francesco Montanari

Research output: Contribution to journalArticleScientificpeer-review

Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume475
Issue number2
Pages (from-to)2787-2808
Number of pages22
ISSN0035-8711
DOIs
Publication statusPublished - Apr 2018
MoE publication typeA1 Journal article-refereed

Fields of Science

  • astro-ph.GA
  • galaxies: clusters: general
  • galaxies: evolution
  • DARK-MATTER HALOES
  • POPULATION SYNTHESIS
  • COSMOS SURVEY
  • HALO OCCUPATION DISTRIBUTION
  • galaxies: elliptical and lenticular, cD
  • STAR-FORMATION RATES
  • SCALING RELATIONS
  • HIGH-REDSHIFT
  • galaxies: groups: general
  • GAS MASS FRACTION
  • CLUSTER GALAXIES
  • X-rays: galaxies: clusters
  • STELLAR MASS
  • galaxies: stellar content
  • 115 Astronomy, Space science

Cite this

Gozaliasl, G., Finoguenov, A., Khosroshahi, H. G., Henriques, B. M. B., Tanaka, M., Ilbert, O., Wuyts, S., McCracken, H. J., & Montanari, F. (2018). Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z <1.3. Monthly Notices of the Royal Astronomical Society, 475(2), 2787-2808. https://doi.org/10.1093/mnras/sty003