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Table 2.
Methods used to determine M⋆ and SFR in this work, in descending order of preference.
| Method | Description |
|---|---|
| 1 | SFR from a combination of FUV and W4 luminosities, thus accounting for both the obscured and the unobscured |
| SF components. Then, M⋆ is derived from W1 luminosities using a mass-to-light ratio (Ψ⋆) that depends on the | |
| specific SFR (see Eq. (24) in Leroy et al. 2019). | |
| 2 | Same as method (1) but using NUV when FUV data are not available. |
| 3 | Same as method (1) but using only WISE W4 luminosities when NUV and FUV data are not available, thus |
| accounting only for the obscured component of the SF. | |
| 4 | SFR from FUV luminosities only, if W4 data are not available, thus accounting only for the unobscured component |
| of the SF. Then M⋆ is derived from W1 data using a constant value for Ψ⋆ = 0.35. | |
| 5 | Same as method (4) but using NUV luminosities when FUV data are not available. |
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