The centre determination of a galaxy cluster from an optical cluster finding algorithm can be offset from theoretical prescriptions or N-body definitions of its host halo centre. These offsets impact the recovered cluster statistics, affecting both richness measurements and the weak lensing shear profile around the clusters. This paper models the centring performance of the redMaPPer cluster finding algorithm using archival X-ray observations of redMaPPer-selected clusters. Assuming the X-ray emission peaks as the fiducial halo centres, and through analysing their offsets to the redMaPPer centres, we find that {˜ } 75± 8 {{ per cent}} of the redMaPPer clusters are well centred and the mis-centred offset follows a Gamma distribution in norma...
International audienceWe perform a joint analysis of the counts and weak lensing signal of redMaPPer...
International audienceContext. The clustering of galaxy clusters links the spatial nonuniformity of ...
Clusters of galaxies are sensitive to the most nonlinear peaks in the cosmic density field. The weak...
The centre determination of a galaxy cluster from an optical cluster finding algorithm can be offset...
We use Dark Energy Survey Year 3 (DES Y3) clusters with archival X-ray data from XMM-Newton and Chan...
We constrain the mass--richness scaling relation of redMaPPer galaxy clusters identified in the Dark...
We constrain the mass-richness scaling relation of redMaPPer galaxy clusters identified in the Dark ...
Counts of galaxy clusters offer a high-precision probe of cosmology, but control of systematic error...
We describe updates to the redMaPPer algorithm, a photometric red-sequence cluster finder specifical...
Locating the centers of dark matter halos is critical for understanding the mass profiles of halos, ...
The location of a galaxy cluster’s centroid is typically derived from observations of the galactic a...
82We use weak-lensing shear measurements to determine the mean mass of optically selected galaxy clu...
International audienceWe perform a joint analysis of the counts and weak lensing signal of redMaPPer...
International audienceContext. The clustering of galaxy clusters links the spatial nonuniformity of ...
Clusters of galaxies are sensitive to the most nonlinear peaks in the cosmic density field. The weak...
The centre determination of a galaxy cluster from an optical cluster finding algorithm can be offset...
We use Dark Energy Survey Year 3 (DES Y3) clusters with archival X-ray data from XMM-Newton and Chan...
We constrain the mass--richness scaling relation of redMaPPer galaxy clusters identified in the Dark...
We constrain the mass-richness scaling relation of redMaPPer galaxy clusters identified in the Dark ...
Counts of galaxy clusters offer a high-precision probe of cosmology, but control of systematic error...
We describe updates to the redMaPPer algorithm, a photometric red-sequence cluster finder specifical...
Locating the centers of dark matter halos is critical for understanding the mass profiles of halos, ...
The location of a galaxy cluster’s centroid is typically derived from observations of the galactic a...
82We use weak-lensing shear measurements to determine the mean mass of optically selected galaxy clu...
International audienceWe perform a joint analysis of the counts and weak lensing signal of redMaPPer...
International audienceContext. The clustering of galaxy clusters links the spatial nonuniformity of ...
Clusters of galaxies are sensitive to the most nonlinear peaks in the cosmic density field. The weak...