Average value of log M_h as a function of M_*. The blue band and the green and dotted black pairs of lines show the 1σ confidence limit obtained from our analysis based on the Sérsic, SerExp, and de Vaucouleurs model, respectively. The solid black line is a measurement from Tinker et al. (2017), obtained from galaxy clustering and abundance matching. Error bars indicate the intrinsic scatter in log M_h. The inner (outer) ticks on the error bars relative to our measurements refer to the 84 (16) percentile of our inference on the scatter parameter σ_h. The inference on the intrinsic scatter obtained with the de Vaucouleurs model is omitted to avoid confusion.