Using ∼100 X-ray selected clusters in the Dark Energy Survey Science Verification data, we constrain the luminosity function (LF) of cluster red-sequence galaxies as a function of redshift. This is the first homogeneous optical/X-ray sample large enough to constrain the evolution of the LF simultaneously in redshift (0.1 < z < 1.05) and cluster mass (13.5≤log10(M200crit)∼<15.0). We pay particular attention to completeness issues and the detection limit of the galaxy sample. We then apply a hierarchical Bayesian model to fit the cluster galaxy LFs via a Schechter function, including its characteristic break (m*) to a faint end power-law slope (α). Our method enables us to avoid known issues in similar analyses based on stacking or binning ...
We present a deep, multicolour (UBI) CCD survey using the Palomar 5‐m telescope of a sample of high ...
The ROSAT-European Southern Observatory (ESO) flux-limited X-ray (REFLEX) galaxy cluster survey and ...
We present the results of Chandra and Suzaku X-ray observations of nine moderate-redshift (0.16 \u3c...
Using ∼100 X-ray selected clusters in the Dark Energy Survey Science Verification data, we constrain...
Using ˜100 X-ray selected clusters in the Dark Energy Survey Science Verification data, we constrain...
Using ∼100 X-ray selected clusters in the Dark Energy Survey Science Verification data, we constrain...
Context. Large area catalogs of galaxy clusters constructed from ROSAT All-Sky Survey provide the ba...
We introduce a galaxy cluster mass observable, μ*, based on the stellar masses of cluster members, a...
We present constraints on the mean matter density, {Omega}{sub m}, normalization of the density fluc...
20Context. Large area catalogs of galaxy clusters constructed from ROSAT All-Sky Survey provide the ...
We use imaging from the first three years of the Dark Energy Survey to characterize the dynamical st...
Indexación: Web of ScienceWe present our study of 19 low X-ray luminosity galaxy clusters (L-X simil...
International audienceContext. Large area catalogs of galaxy clusters constructed from ROSAT All-Sky...
We measure the clustering of DES Year 1 galaxies that are intended to be combined with weak lensing ...
We cross-match and compare characteristics of galaxy clusters identified in observations from two sk...
We present a deep, multicolour (UBI) CCD survey using the Palomar 5‐m telescope of a sample of high ...
The ROSAT-European Southern Observatory (ESO) flux-limited X-ray (REFLEX) galaxy cluster survey and ...
We present the results of Chandra and Suzaku X-ray observations of nine moderate-redshift (0.16 \u3c...
Using ∼100 X-ray selected clusters in the Dark Energy Survey Science Verification data, we constrain...
Using ˜100 X-ray selected clusters in the Dark Energy Survey Science Verification data, we constrain...
Using ∼100 X-ray selected clusters in the Dark Energy Survey Science Verification data, we constrain...
Context. Large area catalogs of galaxy clusters constructed from ROSAT All-Sky Survey provide the ba...
We introduce a galaxy cluster mass observable, μ*, based on the stellar masses of cluster members, a...
We present constraints on the mean matter density, {Omega}{sub m}, normalization of the density fluc...
20Context. Large area catalogs of galaxy clusters constructed from ROSAT All-Sky Survey provide the ...
We use imaging from the first three years of the Dark Energy Survey to characterize the dynamical st...
Indexación: Web of ScienceWe present our study of 19 low X-ray luminosity galaxy clusters (L-X simil...
International audienceContext. Large area catalogs of galaxy clusters constructed from ROSAT All-Sky...
We measure the clustering of DES Year 1 galaxies that are intended to be combined with weak lensing ...
We cross-match and compare characteristics of galaxy clusters identified in observations from two sk...
We present a deep, multicolour (UBI) CCD survey using the Palomar 5‐m telescope of a sample of high ...
The ROSAT-European Southern Observatory (ESO) flux-limited X-ray (REFLEX) galaxy cluster survey and ...
We present the results of Chandra and Suzaku X-ray observations of nine moderate-redshift (0.16 \u3c...