Table 2.
Dust-corrected luminosities and inferred SFRs.
| Line/continuum | Luminosity | SFR (M⊙ yr−1) |
|---|---|---|
| Lyα⋆ | 62 |
|
| [O II] ⋆ | 0.3 |
22 ± 13 |
| Hα (narrow) ⋆ | 1 |
49 |
| Hα (broad) † | 20 ± 1 | |
| L1500, UV** | 30 ± 1 | 12 ± 0.3 |
| L5100, NIR† | 130 |
Notes. Luminosities are given in units of 1043 erg s−1. L1500, UV is the intrinsic luminosity at 1500 Å from the UV continuum power-law fit, corrected for attenuation on the fit of AV = 0.38 ± 0.01 (indicated with a * symbol). L5100, NIR is the luminosity at 5100 Å based on the optical/NIR fit, corrected by AV = 5.61 ± 0.04 (indicated with a † symbol) from the fit. Dust correction for lines is the same as in Table 1.
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