90siWe perform a joint analysis of the counts of redMaPPer clusters selected from the Dark Energy Survey (DES) Y1 data and multi-wavelength follow-up data collected within the 2500 deg$^2$ South Pole Telescope (SPT) SZ survey. The SPT follow-up data, calibrating the richness--mass relation of the optically selected redMaPPer catalog, enable the cosmological exploitation of the DES cluster abundance data. To explore possible systematics related to the modeling of projection effects, we consider two calibrations of the observational scatter on richness estimates: a simple Gaussian model which account only for the background contamination (BKG), and a model which further includes contamination and incompleteness due to projection effects (PRJ)...
80We use measurements from the South Pole Telescope (SPT) Sunyaev–Zel’dovich (SZ) cluster survey in ...
75We present weak-lensing (WL) mass constraints for a sample of massive galaxy clusters detected by ...
82We use weak-lensing shear measurements to determine the mean mass of optically selected galaxy clu...
We perform a joint analysis of the counts of redMaPPer clusters selected from the Dark Energy Survey...
We perform a joint analysis of the counts of redMaPPer clusters selected from the Dark Energy Survey...
136We perform a joint analysis of the counts and weak lensing signal of redMaPPer clusters selected ...
87We implement the first blind analysis of cluster abundance data to derive cosmological constraints...
102We cross-match galaxy cluster candidates selected via their Sunyaev-Zel'dovich effect (SZE) signa...
81We derive cosmological constraints using a galaxy cluster sample selected from the 2500 deg2 SPT-S...
89We describe updates to the redMaPPer algorithm, a photometric red-sequence cluster finder specific...
International audienceWe perform a cross validation of the cluster catalogue selected by the red-seq...
102We constrain the mass-richness scaling relation of redMaPPer galaxy clusters identified in the Da...
We present the first joint analysis of cluster abundances and auto or cross-correlations of three co...
87siThe centre determination of a galaxy cluster from an optical cluster finding algorithm can be of...
We perform a joint analysis of the counts and weak lensing signal of redMaPPer clusters selected fro...
80We use measurements from the South Pole Telescope (SPT) Sunyaev–Zel’dovich (SZ) cluster survey in ...
75We present weak-lensing (WL) mass constraints for a sample of massive galaxy clusters detected by ...
82We use weak-lensing shear measurements to determine the mean mass of optically selected galaxy clu...
We perform a joint analysis of the counts of redMaPPer clusters selected from the Dark Energy Survey...
We perform a joint analysis of the counts of redMaPPer clusters selected from the Dark Energy Survey...
136We perform a joint analysis of the counts and weak lensing signal of redMaPPer clusters selected ...
87We implement the first blind analysis of cluster abundance data to derive cosmological constraints...
102We cross-match galaxy cluster candidates selected via their Sunyaev-Zel'dovich effect (SZE) signa...
81We derive cosmological constraints using a galaxy cluster sample selected from the 2500 deg2 SPT-S...
89We describe updates to the redMaPPer algorithm, a photometric red-sequence cluster finder specific...
International audienceWe perform a cross validation of the cluster catalogue selected by the red-seq...
102We constrain the mass-richness scaling relation of redMaPPer galaxy clusters identified in the Da...
We present the first joint analysis of cluster abundances and auto or cross-correlations of three co...
87siThe centre determination of a galaxy cluster from an optical cluster finding algorithm can be of...
We perform a joint analysis of the counts and weak lensing signal of redMaPPer clusters selected fro...
80We use measurements from the South Pole Telescope (SPT) Sunyaev–Zel’dovich (SZ) cluster survey in ...
75We present weak-lensing (WL) mass constraints for a sample of massive galaxy clusters detected by ...
82We use weak-lensing shear measurements to determine the mean mass of optically selected galaxy clu...