Comparisons of fits with and without Herschel photometry, showing offsets (with–without Herschel) in 7 out of 17 of the inferred stellar parameters plotted against each other. Histograms of the offsets are shown above each column and at the end of the last row. Parameters (left to right, bottom row): diffuse dust attenuation (τ_diffuse), birth-cloud dust attenuation (τ_{birth cloud}), mass-weighted age, stellar mass, diffuse dust index (τ_index), stellar metallicity, and SFR over the last 100 Myr bin (y-axis of bottom row). Blue boxes indicate the percent within 1σ, based on UV–MIR modeling; other indicated percentages refer to the population in the respective quadrant, excluding the 1σ box.