Masses of Sunyaev-Zel'dovich Galaxy Clusters Detected by The Atacama Cosmology Telescope: Stacked Lensing Measurements with Subaru HSC Year 3 data

Abstract

We present a stacked lensing analysis of 96 galaxy clusters selected by the thermal Sunyaev-Zel'dovich (SZ) effect in maps of the cosmic microwave background (CMB). We select foreground galaxy clusters with a \(5\sigma\)-level SZ threshold in CMB observations from the Atacama Cosmology Telescope, while we define background source galaxies for the lensing analysis with secure photometric redshift cuts in Year 3 data of the Subaru Hyper Suprime Cam survey. We detect the stacked lensing signal in the range of \(0.1 < R\, [h^{-1}\mathrm{Mpc}] < 100\) in each of three cluster redshift bins, \(0.092<z\le0.445\), \(0.445<z\le0.695\), and \(0.695<z\le1.180\), with 32 galaxy clusters in each bin. The cumulative signal-to-noise ratios of the lensing signal are \(14.6\), \(12.0\), and \(6.6\), respectively. Using a halo-based forward model, we then constrain statistical relationships between the mass inferred from the SZ observation (i.e. SZ mass) and the total mass derived from our stacked lensing measurements. At the average SZ mass in the cluster sample (\(2.1-2.4\times10^{14}\, h^{-1}M_\odot\)), our likelihood analysis shows that the average total mass differs from the SZ counterpart by a factor of \(1.3 \pm 0.2\), \(1.6 \pm 0.2\), and \(1.6 \pm 0.3\) (\(68\%\)) in the aforementioned redshift ranges, respectively. Our limits are consistent with previous lensing measurements, and we find that the cluster modeling choices can introduce a \(1\sigma\)-level difference in our parameter inferences.