Updated version of Fig. 16 from Sharon et al. (2015), showing various estimates for the enclosed spherical mass of RCS2 J2327 as function of radius. The stars-shaped data points show our weak lensing measurements, recomputed for Ω_m = 0.27 and Ω_Λ = 0.73 as assumed by Sharon et al. (2015). The thick (thin) error bars correspond to our combined statistical and systematic uncertainty without (with) including an additional ~20% intrinsic scatter from cluster triaxiality and correlated large-scale structure. The green squares show SZ mass estimates from Hasselfield et al. (2013). The other mass measurements are described in Sharon et al. (2015) and were derived from Magellan spectroscopic, Chandra X-ray, SZA Sunyaev-Zel’dovich, and CFHT wide-field weak lensing observations, as well as richness measurements, where points with dashed error bars indicate extrapolated results. The shaded grey region shows the 1σ range of spherical NFW mass profiles Sharon et al. (2015) fit to the spherical mass estimates indicated with thick circles.