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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 1.

In the left panel, SSPs with different ages and metallicities are from BC03. The first 10 SSPs have different ages but the same metallicity (solar metallicity), and the last 5 SSPs have the same age (5 Gyr) but different metallicities. They are normalized at 5500 Å, and the ith SSP has been shifted upward i − 1 units. The right panel shows the ratios of the small- to large-scale component of each SSPs, and the ith is shifted upward i − 1 units.

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