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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 A1.

Example of mock spectrum with emission lines. In the left panel, the light-blue line is the mock spectrum without emission lines. The orange line is the best-fit stellar spectrum of the matched spectrum in the MaNGA sample (SDSS/DR14). The green line shows the observed emission lines in the matched MaNGA spectrum. The right panel shows the final mock spectrum with emission lines, which is actually the sum of the blue and green lines in the left panel.

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