Notes. The table provides the following information: cluster ID (Col. 1); coordinates (RA and Dec, Cols. 2 and 3); spectroscopic redshift z_spec (Col. 4); weak-lensing mass log M₂₀₀ and its uncertainty (Cols. 5 and 6); spherically integrated Compton-Y parameter log Y₂₀₀ and its uncertainty (Cols. 7 and 8); richness n_200, WL within the weak-lensing radius, centered on the coordinates given in Cols. 2 and 3 (Cols. 9 and 10); coordinates of the barycenter of the galaxy population (RA and Dec, Cols. 11 and 12); positional offset between the barycenter and the coordinates in Cols. 2 and 3 (Col. 13); and richness n_200, A16 within the radius inferred from galaxy counts, along with its uncertainty (Cols. 14 and 15). Except for O26, for which all quantities have been derived in this paper, coordinates in Columns 2 and 3 are from Oguri et al. (2021), and Columns 4 to 8 are from Paper II. The O26 weak-lensing mass is affected by projection effects. Errors in richness are approximated as Gaussian in this table. Numbers needed to derive the exact distribution of richness errors, used in our fit, are listed in Table ??. The Compton-Y value reported for O40 is the 95% upper limit.