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Spergel, Elinor Medezinski, Hironao Miyatake, I-Non Chiu, Keiichi Umetsu, Masamune Oguri, Neta Bahcall, Nicholas Battaglia, Yen-Ting Lin, Yutaka Komiyama","submitted_at":"2017-06-01T18:00:04Z","abstract_excerpt":"Using $\\sim$140 deg$^2$ Subaru Hyper Suprime-Cam (HSC) survey data, we stack the weak lensing (WL) signal around five Planck clusters found within the footprint. This yields a 15$\\sigma$ detection of the mean Planck cluster mass density profile. The five Planck clusters span a relatively wide mass range, $M_{\\rm WL,500c} = (2-30)\\times10^{14}\\,M_\\odot/h$ with a mean mass of $M_{\\rm WL,500c} = (4.15\\pm0.61)\\times10^{14}\\,M_\\odot/h$. The ratio of the stacked Planck Sunyaev-Zel'dovich (SZ) mass to the stacked WL mass is $ \\langle M_{\\rm SZ}\\rangle/\\langle M_{\\rm WL}\\rangle = 1-b = 0.80\\pm0.14$. 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