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Table 2
Emission-line measurements and star formation rates.
| Galaxy | F(Hα) | N2 | SFRHα |
|
| [10-17 erg-1 cm-2] | [M⊙ yr-1] | [M⊙ yr-1] | ||
| (1) | (2) | (3) | (4) | (5) |
|
|
||||
| 020106882 | 14.0 ± 0.8 | −0.71 ± 0.12 | 13.3 | 38.1 |
| 020116027 | 12.4 ± 2.9 | −1.02 ± 0.15 | 14.7 | 42.2 |
| 020126402 | ... | ... | ... | ... |
| 020147106 | 46.8 ± 5.8 | −0.95 ± 0.14 | 54.3 | 92.1 |
| 020149061 | 20.6 ± 1.6 | ... | 16.0 | 45.9 |
| 020164388 | 24.1 ± 1.3 | −0.86 ± 0.10 | 21.1 | 46.5 |
| 020167131 | ... | ... | ... | ... |
| 020182331 | 15.2 ± 5.0 | ... | 10.5 | 51.1 |
| 020193070 | 6.7 ± 0.9 | −0.56 ± 0.13 | 3.0 | 14.4 |
| 020208482 | 2.6 ± 0.5 | ... | 1.2 | 2.6 |
| 020214655 | 23.3 ± 1.1 | −0.68 ± 0.06 | 10.6 | 51.7 |
| 020217890 | ... | ... | ... | ... |
| 020239133 | 7.8 ± 1.0 | ... | 3.4 | 16.5 |
| 020240675 | 8.5 ± 1.0 | ... | 7.1 | 15.7 |
| 020255799 | 5.8 ± 0.7 | −0.65 ± 0.15 | 2.6 | 12.8 |
| 020261328 | 9.5 ± 0.9 | −1.06 ± 0.48 | 11.2 | 19.0 |
| 020278667 | 2.4 ± 1.3 | ... | 1.1 | 4.2 |
| 020283083 | 13.4 ± 1.0 | −0.70 ± 0.12 | 10.3 | 17.4 |
| 020283830 | 11.0 ± 1.1 | −0.82 ± 0.17 | 10.3 | 50.4 |
| 020294045 | 15.5 ± 2.8 | ... | 6.5 | 14.3 |
| 020306817 | ... | ... | ... | ... |
| 020363717 | 37.4 ± 4.3 | −0.87 ± 0.09 | 31.5 | 53.4 |
| 020370467 | 17.3 ± 2.9 | −0.69 ± 0.11 | 14.6 | 71.2 |
| 020386743 | 17.4 ± 1.7 | −0.91 ± 0.08 | 8.1 | 39.4 |
| 020461235 | 7.5 ± 2.0 | −0.67 ± 0.12 | 3.3 | 9.6 |
| 020461893 | 14.5 ± 1.2 | ... | 6.7 | 14.9 |
| 020465775 | 14.5 ± 2.8 | ... | 12.8 | 62.2 |
| 140083410 | 47.0 ± 3.3 | −0.72 ± 0.08 | 16.8 | 37.1 |
| 140096645 | 55.4 ± 4.2 | −0.25 ± 0.02 | 20.9 | 102.1 |
| 140123568 | 5.8 ± 1.2 | −0.69 ± 0.10 | 2.4 | 11.8 |
| 140137235 | 9.6 ± 2.3 | −0.79 ± 0.13 | 4.4 | 21.6 |
| 140217425 | 104.7 ± 4.9 | −0.44 ± 0.02 | 41.0 | 200.0 |
| 140258511 | 42.5 ± 2.7 | −0.51 ± 0.10 | 30.0 | 146.4 |
| 140262766 | 13.1 ± 5.0 | −0.75 ± 0.15 | 10.0 | 10.0 |
| 140545062 | 29.4 ± 3.3 | −0.75 ± 0.06 | 13.4 | 22.7 |
| 220014252 | 50.3 ± 3.1 | −0.67 ± 0.08 | 40.5 | 197.5 |
| 220015726 | 47.5 ± 6.7 | −0.69 ± 0.04 | 37.0 | 106.4 |
| 220071601 | ... | ... | ... | ... |
| 220148046 | ... | ... | ... | ... |
| 220376206 | 72.4 ± 5.1 | −1.04 ± 0.10 | 51.2 | 249.7 |
| 220386469 | 17.1 ± 2.4 | −1.14 ± 0.16 | 7.5 | 36.5 |
| 220397579 | 65.1 ± 9.1 | −1.07 ± 0.07 | 29.4 | 143.2 |
| 220544103 | 55.0 ± 1.9 | −0.56 ± 0.09 | 52.2 | 117.5 |
| 220544394 | 24.3 ± 1.7 | −0.89 ± 0.07 | 10.3 | 50.1 |
| 220576226 | 31.2 ± 1.6 | −0.69 ± 0.04 | 13.6 | 66.3 |
| 220578040 | 20.5 ± 1.9 | −0.80 ± 0.07 | 9.4 | 20.8 |
| 220584167 | 64.3 ± 1.3 | −0.91 ± 0.10 | 68.6 | 202.6 |
| 220596913 | 30.0 ± 1.0 | ... | 23.2 | 36.1 |
| 910193711 | 32.9 ± 18.4 | −0.68 ± 0.09 | 40.6 | 197.7 |
| 910279515 | 14.9 ± 2.1 | −0.83 ± 0.21 | 14.2 | 69.0 |
Notes. Column 2: Hα flux. Column 3: N2 = log ( [ N ii] 6584/Hα) emission-line ratio. Columns 4 and 5: Hα-based star formation rates (corrected – and not – for dust reddening).
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