We refer readers to Golovich+ (2019, J/ApJS/240/39), where we presented our optical spectroscopic and photometric survey of the 29 systems. In brief, we carried out a ground-based photometric campaign using Subaru/Suprime-Cam imaging in two or three bands (typically g+r, g+i, or g+r+i). We observed 18 of the clusters over four nights with Suprime-Cam on 2013 Jul 13; 2014 Feb 25, 26 and 2015 Sep 12.We also carried out a spectroscopic survey using Keck/DEIMOS spectroscopy over 10 nights between 2013 and 2015. In total 54 slit masks were observed. In Table 2, we detail the radio and X-ray data that will be presented in this paper. See Sections 3.2 and 3.3. (4 data files).