2020/10/23 by Z. L. Wen, J. L. Han
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Cluster (spacecraft) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Photometric redshift #Physics #Redshift #Redshift survey #Stellar, planetary, and galactic studies #astro-ph.CO
paper · pdf · doi:10.1093/mnras/staa3308
16 pages, 18 figures, 2 tables, updated version after proof checking, online data available
openalex publication_date 2020/10/23 · openalex created_date 2020/10/29 · arxiv created 2020/11/19 · arxiv updated 2020/11/20 · openalex updated_date 2026/08/05
ABSTRACT We first present a catalogue of photometric redshifts for 14.68 million galaxies derived from the 7-band photometric data of Hyper Suprime-Cam Subaru Strategic Program and the Wide-field Infrared Survey Explorer using the nearest-neighbour algorithm. The redshift uncertainty is about 0.024 for galaxies of z ≤ 0.7, and steadily increases with redshift to about 0.11 at z ∼ 2. From such a large data set, we identify 21 661 clusters of galaxies, among which 5537 clusters have redshifts z > 1 and 642 clusters have z > 1.5, significantly enlarging the high redshift sample of galaxy clusters. Cluster richness and mass are estimated, and these clusters have an equivalent mass of M500 ≥ 0.7 × 1014 M⊙. We find that the stellar mass of the brightest cluster galaxies (BCGs) in each richness bin does not significantly evolve with redshift. The fraction of star-forming BCGs increases with redshift, but does not depend on cluster mass.