This page provides data products associated with the production of the SZ cluster catalog in Bleem et al. "Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in 5 year data from the SPT-3G Main Survey".

If you have any questions regarding this data set or its use, please contact Lindsey Bleem (lbleem_at_anl_dot_gov).

Catalog in fits file format downloadable from this Argonne National Laboratory box link. Brief description of entries found here.

Footprint of the SPT-3G survey plotted with those of several other multi-wavelength surveys discussed in this work. The footprints are overlaid on a dust map from Planck. (Fig. 1 of Bleem+26).

The expected purity (orange) and number of false detections (green) for the SPT-3G Main field cluster catalog as a function of minimum xi without additional optical follow-up. (Fig. 4 of Bleem+26).

Redshift distribution of the confirmed clusters in the SPT-3G Main field sample confirmed using optical-IR data. (Fig. 8 of Bleem+26).

The mass-redshift distribution of the five-year SPT-3G Main field sample compared to other recent large ICM-selected cluster samples. (Fig. 11 of Bleem+26).

Redshift evolution of the median correlated 220 GHz emission at SPT-3G cluster locations; this emission increases by over an order of magnitude over the redshift range probed by the SPT sample (0.25 < z <2), while the median Compton-y value in each bin is comparable. (Fig. 16 of Bleem+26).