Comparison of our PARAM extinctions with the results obtained by the RJCE method (Zasowski et al. 2013; left panel), isochrone matching (Schultheis et al. 2014; middle panel), and the Pan-STARRS1 dust maps of Schlafly et al. (2014). As before, stars in LRa01 are plotted in blue, while LRc01 stars are plotted in red. The corresponding robust linear fits (using a Huber loss function; see e.g. Ivezić et al. 2013) are shown as solid lines, with the fit coefficients indicated in each panel.