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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 6.

Tests on the effects of the wavelength window size used to define the small- and large-scale components of spectra. Here the standard deviation (σ) of the difference between the output and input E(B − V) values is plotted against the wavelength window size. In each panel, the input value of E(B − V) and the S/N are indicated. The red, green, blue, and yellow lines correspond to spectra in the (a)–(d) regions, respectively. The black line is the result for all the spectra in the four regions.

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