Constraining Gravity Theory Using Weak Lensing Peak Statistics from the Canada-France-Hawaii-Telescope Lensing Survey
arXiv:1607.00184 · doi:10.1103/PhysRevLett.117.051101
Abstract
In this Letter, we report the observational constraints on the Hu-Sawicki theory derived from weak lensing peak abundances, which are closely related to the mass function of massive halos. In comparison with studies using optical or x-ray clusters of galaxies, weak lensing peak analyses have the advantages of not relying on mass-baryonic observable calibrations. With observations from the Canada-France-Hawaii-Telescope Lensing Survey, our peak analyses give rise to a tight constraint on the model parameter for . The CL limit is given WMAP9 priors on . With Planck15 priors, the corresponding result is .
6 pages, 3 figures. Updated to journal version
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