Stellar mass of brightest cluster galaxies

DOI

Using a sample of 98 galaxy clusters recently imaged in the near-infrared with the European Southern Observatory (ESO) New Technology Telescope, WIYN telescope and William Herschel Telescope, supplemented with 33 clusters from the ESO archive, we measure how the stellar mass of the most massive galaxies in the universe, namely brightest cluster galaxies (BCGs), increases with time. Most of the BCGs in this new sample lie in the redshift range 0.2

Identifier
DOI http://doi.org/10.26093/cds/vizier.74602862
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/460/2862
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/460/2862
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/460/2862
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/460/2862
Provenance
Creator Bellstedt S.; Lidman C.; Muzzin A.; Franx M.; Guatelli S.; Hill A.R.,Hoekstra H.; Kurinsky N.; Labbe I.; Marchesini D.; Marsan Z.C.,Safavi-Naeini M.; Sifon C.; Stefanon M.; van de Sande J.; van Dokkum P.,Weigel C.
Publisher CDS
Publication Year 2017
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics