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Arnold, K. Cheung, L. Howe, L. N. Lowry, M. Aguilar Faundez, M. Hasegawa, M. Hazumi, M. Navaroli, M. Silva-Feaver, N. Galitzki, N. Goeckner-Wald, N. Katayama, N. Krachmalnicoff, O. Tajima, R. Stompor, S. Takakura, S. Takatori, T. Elleflot, Y. Chinone, Y. Minami","submitted_at":"2019-03-17T09:26:44Z","abstract_excerpt":"We report a 4.8$\\sigma$ measurement of the cross-correlation signal between the cosmic microwave background (CMB) lensing convergence reconstructed from measurements of the CMB polarization made by the POLARBEAR experiment and the infrared-selected galaxies of the Herschel-ATLAS survey. This is the first measurement of its kind. We infer a best-fit galaxy bias of $b = 5.76 \\pm 1.25$, corresponding to a host halo mass of $\\log_{10}(M_h/M_\\odot) =13.5^{+0.2}_{-0.3}$ at an effective redshift of $z \\sim 2$ from the cross-correlation power spectrum. 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