Constraints on the Richness-Mass Relation and the Optical-SZE Positional Offset Distribution for SZE-Selected Clusters

We cross-match galaxy cluster candidates selected via their Sunyaev-Zel'dovich effect (SZE) signatures in 129.1 deg2 of the South Pole Telescope 2500d SPT-SZ survey with optically identified clusters selected from the Dark Energy Survey science verification data. We identify 25 clusters between 0.1 ≲ z ≲ 0.8 in the union of the SPT-SZ and redMaPPer (RM) samples. RM is an optical cluster finding algorithm that also returns a richness estimate for each cluster. We model the richness lambda-mass relation with the following function ∝ Blambdaln M500 + Clambdaln E(z) and use SPT-SZ cluster masses and RM richnesses lambda to constrain the parameters. We find B_lambda = 1.14^{+0.21}_{-0.18} and C_lambda =0.73^{+0.77}_{-0.75}. The associated scatter in mass at fixed richness is sigma _{ln M|lambda } = 0.18^{+0.08}_{-0.05} at a characteristic richness lambda = 70. We demonstrate that our model provides an adequate description of the matched sample, showing that the fraction of SPT-SZ-selected clusters with RM counterparts is consistent with expectations and that the fraction of RM-selected clusters with SPT-SZ counterparts is in mild tension with expectation. We model the optical-SZE cluster positional offset distribution with the sum of two Gaussians, showing that it is consistent with a dominant, centrally peaked population and a subdominant population characterized by larger offsets. We also cross-match the RM catalogue with SPT-SZ candidates below the official catalogue threshold significance xi = 4.5, using the RM catalogue to provide optical confirmation and redshifts for 15 additional clusters with xi ∈ [4, 4.5].