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- W3100306509 abstract "Aims. By means of the r -band luminosity function (LF) of galaxies in a sample of about 4000 clusters detected by the cluster finder AMICO in the KiDS-DR3 area of about 400 deg 2 , we studied the evolution with richness and redshift of the passive evolving (red), star-forming (blue), and total galaxy populations. This analysis was performed for clusters in the redshift range [0.1, 0.8] and in the mass range [10 13 M ⊙ , 10 15 M ⊙ ]. Methods. To compute LFs, we binned the luminosity distribution in magnitude and statistically subtracted the background. Then, we divided the cluster sample in bins of both redshift and richness/mass. We stacked LF counts in each 2D bin for the total, red, and blue galaxy populations; finally, we fitted the stacked LF with a Schechter function and studied the trend of its parameters with redshift and richness/mass. Results. We found a passive evolution with z for the bright part of the LF for the red and total populations and no significant trends for the faint galaxies. The mass/richness dependence is clear for the density parameter Φ ⋆ , increasing with richness, and for the total population faint end, which is shallower in the rich clusters." @default.
- W3100306509 created "2020-11-23" @default.
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- W3100306509 date "2020-12-21" @default.
- W3100306509 modified "2023-10-18" @default.
- W3100306509 title "AMICO galaxy clusters in KiDS-DR3: Evolution of the luminosity function between<i>z</i>= 0.1 and<i>z</i>= 0.8" @default.
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- W3100306509 doi "https://doi.org/10.1051/0004-6361/202039259" @default.
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