@article{oai:nagoya.repo.nii.ac.jp:00028388,
 author = {Miyatake, Hironao and Battaglia, Nicholas and Hilton, Matt and Medezinski, Elinor and Nishizawa, Atsushi J. and More, Surhud and Aiola, Simone and Bahcall, Neta and Bond, J. Richard and Calabrese, Erminia and Choi, Steve K. and Devlin, Mark J. and Dunkley, Joanna and Dunner, Rolando and Fuzia, Brittany and Gallardo, Patricio and Gralla, Megan and Hasselfield, Matthew and Halpern, Mark and Hikage, Chiaki and Hill, J. Colin and Hincks, Adam D. and Hložek, Renée and Huffenberger, Kevin and Hughes, John P. and Koopman, Brian and Kosowsky, Arthur and Louis, Thibaut and Madhavacheril, Mathew S. and McMahon, Jeff and Mandelbaum, Rachel and Marriage, Tobias A. and Maurin, Loïc and Miyazaki, Satoshi and Moodley, Kavilan and Murata, Ryoma and Naess, Sigurd and Newburgh, Laura and Niemack, Michael D. and Nishimichi, Takahiro and Okabe, Nobuhiro and Oguri, Masamune and Osato, Ken and Page, Lyman and Partridge, Bruce and Robertson, Naomi and Sehgal, Neelima and Sherwin, Blake and Shirasaki, Masato and Sievers, Jonathan and Sifón, Cristóbal and Simon, Sara and Spergel, David N. and Staggs, Suzanne T. and Stein, George and Takada, Masahiro and Trac, Hy and Umetsu, Keiichi and Engelen, Alex van and Wollack, Edward J.},
 issue = {1},
 journal = {The Astrophysical Journal},
 month = {Apr},
 note = {We present weak-lensing measurements using the first-year data from the Hyper Suprime-Cam Strategic Survey Program on the Subaru telescope for eight galaxy clusters selected through their thermal Sunyaev–Zel'dovich (SZ) signal measured at 148 GHz with the Atacama Cosmology Telescope Polarimeter experiment. The overlap between the two surveys in this work is 33.8 square degrees, before masking bright stars. The signal-to-noise ratio of individual cluster lensing measurements ranges from 2.2 to 8.7, with a total of 11.1 for the stacked cluster weak-lensing signal. We fit for an average weak-lensing mass distribution using three different profiles, a Navarro–Frenk–White profile, a dark-matter-only emulated profile, and a full cosmological hydrodynamic emulated profile. We interpret the differences among the masses inferred by these models as a systematic error of 10%, which is currently smaller than the statistical error. We obtain the ratio of the SZ-estimated mass to the lensing-estimated mass (the so-called hydrostatic mass bias 1−b) of ${0.74}_{-0.12}^{+0.13}$, which is comparable to previous SZ-selected clusters from the Atacama Cosmology Telescope and from the Planck Satellite. We conclude with a discussion of the implications for cosmological parameters inferred from cluster abundances compared to cosmic microwave background primary anisotropy measurements.},
 title = {Weak-lensing Mass Calibration of ACTPol Sunyaev–Zel’dovich Clusters with the Hyper Suprime-Cam Survey},
 volume = {875},
 year = {2019}
}