CCCP and MENeaCS: (updated) weak-lensing masses for 100 galaxy clusters

Large area surveys have detected significant samples of galaxy clusters that can be used to constrain cosmological parameters, provided that the masses of the clusters are measured robustly. To improve the calibration of cluster masses using weak gravitational lensing we present new results for 48 clusters at $0.05

Keywords:

• Astrophysics
• Galaxy cluster
• Physics
• Weak gravitational lensing

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