Image Details
Caption: Figure 12.
Top: distribution of the relative difference of E(B − V) between the fitted model curves of Calzetti, CCM, and SMC (panels from left to right) and the measured curve. Plotted in different colors are results for spaxels at different radii, as indicated. Bottom: distribution of the rms scatter of the fitted curves around the measured one.
© 2020. The Author(s). Published by the American Astronomical Society.