Constraining $f(R)$ Gravity Theory Using Weak Lensing Peak Statistics   from the Canada-France-Hawaii-Telescope Lensing Survey
  In this Letter, we report the observational constraints on the Hu-Sawicki $f(R)$ 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 $|f_{R0}|$ for $n=1$. The $95\%$ CL limit is $\log_{10}|f_{R0}| < -4.82$ given WMAP9 priors on $(\Omega_{\rm m}, A_{\rm s})$. With Planck15 priors, the corresponding result is $\log_{10}|f_{R0}| < -5.16$. 
Xiangkun Liu, Baojiu Li, Gong-Bo Zhao, Mu-Chen Chiu, Wei Fang,   Chuzhong Pan, Qiao Wang, Wei Du, Shuo Yuan, Liping Fu, and ...
astro-ph.CO