Constraints on the Richness-Mass Relation and the Optical-SZE Positional Offset Distribution for SZE-Selected Clusters
arXiv:1506.07814 · doi:10.1093/mnras/stv2141
Abstract
We cross-match galaxy cluster candidates selected via their Sunyaev-Zel'dovich effect (SZE) signatures in 129.1 deg of the South Pole Telescope 2500d SPT-SZ survey with optically identified clusters selected from the Dark Energy Survey (DES) science verification data. We identify 25 clusters between 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 -mass relation with the following function and use SPT-SZ cluster masses and RM richnesses to constrain the parameters. We find and . The associated scatter in mass at fixed richness is at a characteristic richness . 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 sub-dominant population characterized by larger offsets. We also cross-match the RM catalog with SPT-SZ candidates below the official catalog threshold significance , using the RM catalog to provide optical confirmation and redshifts for additional low- SPT-SZ candidates.In this way, we identify 15 additional clusters with over the redshift regime explored by RM in the overlapping region between DES science verification data and the SPT-SZ survey.
15 pages, 8 Figures, submitted to MNRAS