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Estimating Dust Attenuation from Galactic Spectra. I. Methodology and Tests

  • Authors: Niu Li, Cheng Li, Houjun Mo, Jian Hu, Shuang Zhou, and Cheng Du

2020 The Astrophysical Journal 896 38.

  • Provider: AAS Journals

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.

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