Table 9.
Comparison of SFR estimates for LARS galaxies.
| ID | SFRHα | SFR22 μm | SFR[C II] | SFR[O I] | SFRTIR |
|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) |
| 1 | 6.5 | 4.6 ± 0.12 | – | – |
 |
| 2 | 1.4 | 0.2 ± 0.06 | 0.4 ± 0.2 | < 2.3 |
 |
| 3 | 26.3 | 105.7 ± 0.3 | 35.5 ± 0.8 | 73 ± 3 |
 |
| 4 | 6.1 | 5.2 ± 0.15 | – | – |
 |
| 5 | 5.8 | 2.0 ± 0.1 | 29 ± 5 | – |
 |
| 6 | 0.6 | – | – | – |
 |
| 7 | 9.3 | 4.6 ± 0.2 | – | – |
 |
| 8 | 36.8 | 31.0 ± 0.32 | 81 ± 13 | – |
 |
| 9 | 40.7 | 24.7 ± 0.44 | 33.4 ± 0.6 | 34 ± 3 |
 |
| 10 | 5.6 | 1.9 ± 0.3 | – | – |
 |
| 11 | 30.5 | 28.4 ± 1.01 | 203 ± 12 | – |
 |
| 12 | 97.0 | 12.7 ± 0.72 | 8.7 ± 1.2 | 16 ± 4 |
 |
| 13 | 64.8 | 66.5 ± 3.02 | 40.5 ± 4.1 | 54 ± 10 |
 |
| 14 | 24.8 | 7.0 ± 2.13 | – | – |
 |
Notes. The SFRs are given in units of M⊙ yr−1. The LARS ID is shown in Col. 1. Previously published SFRs from extinction-corrected Hα (Hayes et al. 2014) are found in Col. 2. New SFR estimates from WISE 22 μm, [C II]158 μm, [O I]63 μm, and total infrared luminosities are given in Cols. 3–6. Total infrared luminosities in Col. 6 are used for all analysis (KS plots etc.) in this paper.
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