Table 2.
Summary of coefficients to convert the luminosity in different bands into SFR.
| Coefficient C | Band(s) | log10(C) | Reference |
|---|---|---|---|
| [M⊙ yr−1/(erg s−1)] | |||
| CFUV | FUV | −43.42 | (1) |
 |
FUV+W4 | −42.73 | (1) |
 |
FUV+W4 | −42.91 | (2)⋆, K12 |
| CHα | Hα | −41.26 | (3), K12 |
 |
Hα+W4 | −42.86 | (3)⋆ |
 |
Hα+W4 | −43.05 | (4)⋆, K12 |
Notes. Coefficients are defined in Eqs. (3)–(5). An asterisk implies that the original calibration was derived with Spitzer MIPS and was revised downward by 0.08 dex for application with 22 μm WISE W4.
References. 1: Leroy et al. (2019), 2: Hao et al. (2011), 3: Calzetti et al. (2007), 4: Kennicutt et al. (2009), K12: Kennicutt & Evans (2012).
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