Data to reproduce the results of the paper Thermal SZ Effect in the CGM- II: dependence on star formation

In our paper, we use a publicly available galaxy catalog, Compton-y maps, and simulated datasets. The stacked Compton-y profiles, results of thermal pressure modeling, and derived quantities from those are provided here in FITS files. The description of each file is provided in the headers. The files would help reproduce Figures 5,7,8,9, and the figures in the appendix. In the rest of the figures, we use publicly available data that is appropriately cited throughout the paper.