Resulting posterior distributions on Δ_M for different runs. We show the LEPHARE-NL stellar mass correction results in orange and average stellar mass correction results in green, compared to the fit using the original stellar masses from Betoule et al. (2014). Vertical lines indicate the best-fit value for each configuration. We find that the fiducial model has a slightly larger value for Δ_M than either of the mass-corrected models, being very close to the best-fit value for the LEPHARE-NL correction model. Nevertheless, the resulting distributions for both mass-corrected models are similar.