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We present results from cross-correlating Planck CMB lensing maps with the Sloan Digital Sky Survey (SDSS) galaxy lensing shape catalog and BOSS galaxy catalogs. For galaxy position vs. CMB lensing cross-correlations, we measure the convergence signal around the galaxies in configuration space, using the BOSS LOWZ (z0. 30) and CMASS (z0. 57) samples. With fixed Planck 2015 cosmology, doing a joint fit with the galaxy clustering measurement, for the LOWZ (CMASS) sample we find a galaxy bias bg=1. 750. 04 (1. 95 0. 02) and galaxy-matter cross-correlation coefficient r₂₂=1. 00. 2 (0. 8 0. 1) using 20<rₚ<70h^-1Mpc, consistent with results from galaxy-galaxy lensing. Using the same scales and including the galaxy-galaxy lensing measurements, we constrain ₘ=0. 2840. 024 and relative calibration bias between the CMB lensing and galaxy lensing to be b_=0. 82^+0. 15-₀. ₁₄. The combination of galaxy lensing and CMB lensing also allows us to measure the cosmological distance ratios (with zₗ0. 3, zₛ0. 5) R=Dₛ D₋, *D_* D₋, ₒ=2. 680. 29, consistent with predictions from the Planck 2015 cosmology (R=2. 35). We detect the galaxy position-CMB convergence cross-correlation at small scales, rₚ<1h^-1Mpc, and find consistency with lensing by NFW halos of mass Mₕ10^13h^-1M_. Finally, we measure the CMB lensing-galaxy shear cross-correlation, finding an amplitude of A=0. 760. 23 (zₑff=0. 35, <2^) with respect to Planck 2015 CDM predictions (1-level consistency). We do not find evidence for relative systematics between the CMB and SDSS galaxy lensing.
Singh et al. (Thu,) studied this question.