Battaglia, N.Leauthaud, A.Miyatake, H.Hasselfield, M.Grallad, M. B.Allison, R.Bond, J. R.Calabrese, E.Crichton, D.Devlin, M. J.Dunkley, J.Duenner, R.Erben, T.Ferrara, S.Halpern, M.Hilton, M.Hill, J. C.Hincks, A. D.Hlozek, R.Huffenberger, K. M.Hughes, J. P.Kneib, J. P.Kosowsky, A.Makler, M.Marriage, T. A.Menanteaus, F.Miller, L.Moodley, K.Moraesv, B.Niemack, M. D.Page, L.Shan, H.Sehgal, N.Sherwin, B. D.Sievers, J. L.Sifon, C.Spergel, D. N.Staggs, S. T.Taylor, J. E.Thornton, R.Van Waerbekek, L.Wollackag, E. J.2017-01-242017-01-242017-01-24201610.1088/1475-7516/2016/08/013https://infoscience.epfl.ch/handle/20.500.14299/133819WOS:000389859100005Mass calibration uncertainty is the largest systematic effect for using clusters of galaxies to constrain cosmological parameters. We present weak lensing mass measurements from the Canada-France-Hawaii Telescope Stripe 82 Survey for galaxy clusters selected through their high signal-to-noise thermal Sunyaev-Zeldovich (tSZ) signal measured with the Atacama Cosmology Telescope (ACT). For a sample of 9 ACT clusters with a tSZ signal-to-noise greater than five the average weak lensing mass is (4.8 +/- 0.8) x 10(14) M-circle dot, consistent with the tSZ mass estimate of (4.70 +/- 1.0) x 10(14) M-circle dot which assumes a universal pressure profile for the cluster gas. Our results are consistent with previous weak-lensing measurements of tSZ-detected clusters from the Planck satellite. When comparing our results, we estimate the Eddington bias correction for the sample intersection of Planck and weak-lensing clusters which was previously excluded.galaxy clustersgravitational lensingSunyaev-Zeldovich effecttext::journal::journal article::research article