22siThe COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the largest flux limited sample of X-ray clusters at 0.35 < z < 0.65. It was selected from ROSAT data in the 10,000 square degrees of overlap with BOSS, mapping a total number of 2770 high-z galaxy clusters. We present here the full results of the CFHT CODEX program on cluster mass measurement, including a reanalysis of CFHTLS Wide data, with 25 individual lensing-constrained cluster masses. We employ lensfit shape measurement and perform a conservative colour-space selection and weighting of background galaxies. Using the combination of shape noise and an analytic covariance for intrinsic variations of cluster profiles at fixed mass due to large scale structure, misc...
We present the weak-lensing analysis of 279 CODEX clusters using imaging data from 4200 deg(2) of th...
We present the weak-lensing analysis of 279 CODEX clusters using imaging data from 4200 deg(2) of th...
International audienceWe present a stacked weak-lensing analysis of 27 richness selected galaxy clus...
The COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the largest flux limited sampl...
The COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the largest flux limited sampl...
International audienceThe COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the larg...
International audienceThe COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the larg...
International audienceThe COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the larg...
International audienceThe COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the larg...
International audienceThe COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the larg...
International audienceWe present the weak-lensing analysis of 279 CODEX clusters using imaging data ...
International audienceWe present the weak-lensing analysis of 279 CODEX clusters using imaging data ...
International audienceWe present the weak-lensing analysis of 279 CODEX clusters using imaging data ...
International audienceWe present the weak-lensing analysis of 279 CODEX clusters using imaging data ...
We present a stacked weak-lensing analysis of 27 richness selected galaxy clusters at 0.40 <= z <= 0...
We present the weak-lensing analysis of 279 CODEX clusters using imaging data from 4200 deg(2) of th...
We present the weak-lensing analysis of 279 CODEX clusters using imaging data from 4200 deg(2) of th...
International audienceWe present a stacked weak-lensing analysis of 27 richness selected galaxy clus...
The COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the largest flux limited sampl...
The COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the largest flux limited sampl...
International audienceThe COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the larg...
International audienceThe COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the larg...
International audienceThe COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the larg...
International audienceThe COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the larg...
International audienceThe COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the larg...
International audienceWe present the weak-lensing analysis of 279 CODEX clusters using imaging data ...
International audienceWe present the weak-lensing analysis of 279 CODEX clusters using imaging data ...
International audienceWe present the weak-lensing analysis of 279 CODEX clusters using imaging data ...
International audienceWe present the weak-lensing analysis of 279 CODEX clusters using imaging data ...
We present a stacked weak-lensing analysis of 27 richness selected galaxy clusters at 0.40 <= z <= 0...
We present the weak-lensing analysis of 279 CODEX clusters using imaging data from 4200 deg(2) of th...
We present the weak-lensing analysis of 279 CODEX clusters using imaging data from 4200 deg(2) of th...
International audienceWe present a stacked weak-lensing analysis of 27 richness selected galaxy clus...