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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 A2.

Tests on mock spectra generated with continuous SFH, with (open histograms) or without (filled histograms) including emission lines. Panels from left to right correspond to different E(B − V), and panels from top to bottom correspond to different S/Ns, as indicated. In each panel, the histograms show the distribution of the difference between the output and input value of E(B − V), referred to as ΔE(B − V). Indicated in each panel are the mean value and standard deviation of ΔE(B − V) for both the filled (black) and open (blue) histograms.

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