AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence

@article{Radovich2020AMICOGC,
  title={AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence},
  author={Mario Radovich and Crescenzo Tortora and Fabio Bellagamba and Matteo Maturi and Lauro Moscardini and E. Puddu and Mauro Roncarelli and Nivya Roy and Sandro Bardelli and Federico Marulli and Mauro Sereno and Fedor I. Getman and Nicola R. Napolitano},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2020},
  volume={498},
  pages={4303-4315}
}
A catalogue of galaxy clusters was obtained in an area of 414 sq deg up to a redshift $z\sim0.8$ from the Data Release 3 of the Kilo-Degree Survey (KiDS-DR3), using the Adaptive Matched Identifier of Clustered Objects (AMICO) algorithm. The catalogue and the calibration of the richness-mass relation were presented in two companion papers. Here we describe the selection of the cluster central galaxy and the classification of blue and red cluster members, and analyze the main cluster properties… 
1 Citations
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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

References

SHOWING 1-10 OF 93 REFERENCES
amico galaxy clusters in KiDS-DR3: sample properties and selection function
We present the first catalogue of galaxy cluster candidates derived from the third data release of the Kilo Degree Survey (KiDS-DR3). The sample of clusters has been produced using the Adaptive
AMICO galaxy clusters in KiDS-DR3: weak lensing mass calibration
We present the mass calibration for galaxy clusters detected with the AMICO code in KiDS DR3 data. The cluster sample comprises $\sim$ 7000 objects and covers the redshift range 0.1 < $z$ < 0.6. We
Searching for galaxy clusters in the Kilo-Degree Survey
In this paper, we present the tools used to search for galaxy clusters in the Kilo Degree Survey (KiDS), and our first results. The cluster detection is based on an implementation of the optimal
RedMaPPer: Evolution and Mass Dependence of the Conditional Luminosity Functions of Red Galaxies in Galaxy Clusters
We characterize the luminosity distribution, halo mass dependence, and redshift evolution of red galaxies in galaxy clusters using the SDSS Data Release 8 RedMaPPer cluster sample. We propose a
Cosmological Interpretation of the Color–Magnitude Diagrams of Galaxy Clusters
We investigate the color-magnitude diagram (CMD) of cluster galaxies in the hierarchical $\Lambda$-CDM cosmological scenario using both single stellar populations and simple galaxy models. First, we
Evolution of galaxy size–stellar mass relation from the Kilo-Degree Survey
We have obtained structural parameters of about 340,000 galaxies from the Kilo Degree Survey (KiDS) in 153 square degrees of data release 1, 2 and 3. We have performed a seeing convolved 2D single
The Galaxy Content of SDSS Clusters and Groups
Imaging data from the Sloan Digital Sky Survey are used to characterize the population of galaxies in groups and clusters detected with the MaxBCG algorithm. We investigate the dependence of
Cosmological Simulations of Galaxy Clusters
We review recent progress in the description of the formation and evolution of galaxy clusters in a cosmological context by using state-of-art numerical simulations. We focus our presentation on the
Substructure and dynamical state of 2092 rich clusters of galaxies derived from photometric data
Dynamical state of galaxy clusters is closely related to the ir observational properties in X-ray, optical and radio wavelengths. We develop a method to diagnose the substructure and dynamical state
Evolution of the cluster optical galaxy luminosity function in the CFHTLS: breaking the degeneracy between mass and redshift
Obtaining large samples of galaxy clusters is important for cosmology, since cluster counts as a function of redshift and mass can constrain the parameters of our Universe. They are also useful to
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