Weak-lensing mass calibration of redMaPPer galaxy clusters in Dark Energy Survey Science Verification data
We use weak-lensing shear measurements to determine the mean mass of optically selected galaxy clusters in Dark Energy Survey Science Verification data. In a blinded analysis, we split the sample of more than 8000 redMaPPer clusters into 15 subsets, spanning ranges in the richness parameter 5 <=...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Language: | en |
Published: |
OXFORD UNIV PRESS
2017
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Online Access: | http://hdl.handle.net/10150/625502 http://arizona.openrepository.com/arizona/handle/10150/625502 |