1959 massive galaxy clusters at high redshifts

DOI

We identify a sample of 1959 massive clusters of galaxies in the redshift range of 0.70.75. By comparing them with clusters at lower redshifts, we confirm that richer clusters host more luminous brightest cluster galaxies (BCGs) also at high redshifts, and that the fraction of blue galaxies is larger in clusters at higher redshifts. A small fraction of BCGs show ongoing star formation or active nuclei. The number density profile of member galaxies in stacked samples of clusters shows no significant redshift evolution.

Cone search capability for table J/MNRAS/481/4158/table1 (The 1959 massive clusters of galaxies identified from the SDSS and WISE)

Cone search capability for table J/MNRAS/481/4158/tablea1 (Parameters of 45 clusters with known mass (M500) from literature)

Identifier
DOI http://doi.org/10.26093/cds/vizier.74814158
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/481/4158
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/481/4158
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/481/4158
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/481/4158
Provenance
Creator Wen Z.L.; Han J.L.
Publisher CDS
Publication Year 2022
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