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Table 1.
Parameters for the SED fitting.
| Parameters | Symbol | Range |
|---|---|---|
| Mass fraction of PAH | qPAH | 0.47 |
| Minimum radiation field | Umin | 17.0 |
| Power-law slope dU/dMDust ∼ Uα | α | 2.4 |
| Dust fraction heated by starlight | γ | 0.54 |
| e-folding timescale [Myr] | τmain | 500 |
| Age of main stellar population [Myr] | Agemain | 101 log values in [2–1200] |
| Burst | fburst | No burst |
| Metallicity of the single stellar populations | Z | 0.004 |
| Ionization parameter | log U | −2.5, −2.0, −1.5 |
| Color excess | E_BV | 101 log values in [0.01, 1.0] |
| Power-law slope | δ | 0.0 |
| IMF slope | ξ | Chabrier (2003), TH (1.35, 1.5, 1.8) |
Notes. Parameters for the SED fitting of the galaxies adopted from Burgarella et al. (2022). The parameters for dust emission are derived from stacked IR template.
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