International audienceThe 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 |${\sim } 75\pm 8 {{\ \rm per\ cent}}$| of the redMaPPer clusters are well centred and the mis-centred offset ...
We present the calibration of the Dark Energy Survey Year 3 (DES Y3) weak lensing (WL) source galaxy...
International audienceSplashback refers to the process of matter that is accreting onto a dark matte...
We cross-match and compare characteristics of galaxy clusters identified in observations from two sk...
The centre determination of a galaxy cluster from an optical cluster finding algorithm can be offset...
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 perform a joint analysis of the counts and weak lensing signal of redMaPPer clusters selected fro...
Using archival X-ray observations and a lognormal population model, we estimate constraints on the i...
We perform a joint analysis of the counts and weak lensing signal of redMaPPer clusters selected fro...
Using archival X-ray observations and a log-normal population model, we estimate constraints on the ...
International audienceWe describe updates to the redMaPPer algorithm, a photometric red-sequence clu...
We describe updates to the redMaPPer algorithm, a photometric red-sequence cluster finder specifical...
International audienceWeak lensing source galaxy catalogues used in estimating the masses of galaxy ...
International audienceWe use weak-lensing shear measurements to determine the mean mass of optically...
Weak lensing source galaxy catalogues used in estimating the masses of galaxy clusters can be heavil...
We present the calibration of the Dark Energy Survey Year 3 (DES Y3) weak lensing (WL) source galaxy...
International audienceSplashback refers to the process of matter that is accreting onto a dark matte...
We cross-match and compare characteristics of galaxy clusters identified in observations from two sk...
The centre determination of a galaxy cluster from an optical cluster finding algorithm can be offset...
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 perform a joint analysis of the counts and weak lensing signal of redMaPPer clusters selected fro...
Using archival X-ray observations and a lognormal population model, we estimate constraints on the i...
We perform a joint analysis of the counts and weak lensing signal of redMaPPer clusters selected fro...
Using archival X-ray observations and a log-normal population model, we estimate constraints on the ...
International audienceWe describe updates to the redMaPPer algorithm, a photometric red-sequence clu...
We describe updates to the redMaPPer algorithm, a photometric red-sequence cluster finder specifical...
International audienceWeak lensing source galaxy catalogues used in estimating the masses of galaxy ...
International audienceWe use weak-lensing shear measurements to determine the mean mass of optically...
Weak lensing source galaxy catalogues used in estimating the masses of galaxy clusters can be heavil...
We present the calibration of the Dark Energy Survey Year 3 (DES Y3) weak lensing (WL) source galaxy...
International audienceSplashback refers to the process of matter that is accreting onto a dark matte...
We cross-match and compare characteristics of galaxy clusters identified in observations from two sk...