Table B.2.
Results from the analysis of high-resolution spectroscopy of the sample.
| Target | S/NHα | S/N[OIII] | FWHMHα | FWHM[OIII] | fout, Hα | fout, [OIII] |
|---|---|---|---|---|---|---|
| [km/s] | [km/s] | |||||
| 2MASSJ00114318+1428010 | 107 | 11 | 92 ± 1.5 | 90 ± 11 | 0.2 ± 0.09 | - |
| AGC244381 | 10 | - | 70 ± 14 | - | - | - |
| IC159 | 36 | 7 | 50 ± 5 | 100 ± 20 | - | - |
| IC5292 | 59 | - | 60 ± 3 | - | - | - |
| LEDA1278497 | 22 | 4 | 110 ± 6 | 100 ± 40 | - | - |
| LEDA1397680 | 82 | - | 91 ± 1.2 | - | - | - |
| LEDA1417541 | - | - | - | - | - | - |
| LEDA1439867 | - | 15 | - | 70 ± 6 | - | - |
| LEDA1446233 | - | - | - | - | - | - |
| LEDA1452135 | - | - | - | - | - | - |
| LEDA1464874 | 7 | - | 70 ± 17 | - | - | - |
| LEDA3091160 | 44 | 8 | 100 ± 7 | 80 ± 18 | - | - |
| LEDA3127469 | 39 | - | 40 ± 5 | - | - | - |
| LEDA3530 | 164 | 23 | 72 ± 1.1 | 90 ± 3 | 0.1 ± 0.04 | - |
| LEDA49155 | - | 8 | - | 100 ± 17 | - | - |
| MCG+00-34-035 | - | - | - | - | - | - |
| NGC7401 | 13 | - | 80 ± 10 | - | - | - |
| NGC99 | 30 | - | 60 ± 5 | - | - | - |
| SDSSJ002048.58+141327.8 | 86 | 13 | 118 ± 1.5 | 120 ± 5 | - | - |
| SDSSJ011437.36+011053.4 | - | - | - | - | - | - |
| SDSSJ120108.03+152353.6 | - | - | - | - | - | - |
| SDSSJ135906.39+175604.9 | - | 11 | - | 110 ± 11 | - | - |
| SDSSJ140317.75+100340.3 | 81 | 25 | 60 ± 4 | 70 ± 2 | - | - |
| UGC10005 | - | - | - | - | - | - |
| UGC11992 | - | - | - | - | - | - |
| UGC272 | 7 | - | < 60 | - | - | - |
| UGC6838 | 25 | - | 100 ± 5 | - | - | - |
| UGC9359 | - | - | - | - | - | - |
| Z38-48 | 37 | 4 | 80 ± 3 | 100 ± 40 | - | - |
| Z383-30 | 25 | - | 60 ± 6 | - | - | - |
| Z386-19 | 25 | - | 60 ± 5 | - | - | - |
| Z429-16 | 90 | 22 | 80 ± 1.5 | 90 ± 4 | 0.3 ± 0.11 | - |
| Z429-21 | 50 | 6 | 80 ± 2 | < 110 | - | - |
| Z436-34 | 22 | - | 60 ± 6 | - | - | - |
| Z68-62 | 17 | 5 | 70 ± 7 | 100 ± 40 | - | - |
| Z72-15 | 14 | - | 70 ± 9 | - | - | - |
| Z80-42 | 35 | 6 | 70 ± 4 | 80 ± 16 | - | - |
| Z97-38 | - | - | - | - | - | - |
| LEDA1389480 | 41 | 11 | 70 ± 3 | 70 ± 5 | - | - |
| NGC2741 | 530 | - | 81 ± 1.1 | - | - | - |
| MRK802 | 720 | - | 79 ± 0.6 | - | 0.31 ± 0.015 | - |
| LEDA213877 | - | - | - | - | - | - |
| MRK444 | 510 | 40 | 102 ± 0.7 | 103 ± 0.8 | 0.12 ± 0.019 | < 0.5 |
| Z102-75 | 24 | - | 100 ± 3 | - | - | - |
| NGC2607 | 4 | 4 | 20 ± 13 | 50 ± 20 | - | - |
| MRK399 | 229 | 26 | 118 ± 0.8 | 122 ± 1.3 | - | < 0.4 |
| LEDA31379 | 17 | - | 100 ± 5 | - | 0.4 ± 0.12 | - |
| MRK58 | 159 | 4 | 88 ± 0.9 | 130 ± 19 | 0.2 ± 0.04 | - |
| LEDA3998175 | - | - | - | - | - | - |
| Z65-27 | 88 | 32 | 80 ± 1.6 | 114 ± 1.7 | 0.4 ± 0.06 | 0.4 ± 0.16 |
| UGC7017 | 104 | 5 | 140 ± 1.5 | 110 ± 17 | 0.2 ± 0.08 | - |
| LEDA86470 | 160 | 17 | 86 ± 0.7 | 110 ± 3 | 0.2 ± 0.07 | - |
Notes. Columns two and three list the emission line FWHM (deconvolved from instrumental resolution) for Hα and [OIII] derived from the single-component fit to the high-resolution spectroscopy where the fit was successful. Columns four and five show the ratio of flux in outflow-like fit components to the total flux in the emission line derived from the multi-component fit to the high-resolution spectroscopy for galaxies in which the best-fit model has outflow-like components (see Section 5.4). Galaxies in the upper section of the table were observed with NTT/EFOSC2 and those in the lower part with TNG/DOLORES.
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