Table 3
Derived H I properties from the Lyman series absorption lines.
| Galaxy name | EB-V | log (NH I) | b | v | Cf fits | Cf depth | Cf final |
|---|---|---|---|---|---|---|---|
| [log(cm−2)] | [km s−1] | [km s−1] | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| J0921+4509 | 0.222 ± 0.015 | 17.94 ± 3.22 | 95 ± 49 | –56 ± 13 | 0.754 ± 0.111 | 0.769 ± 0.116 | 0.761 ± 0.080 |
| J1503+3644 | 0.274 ± 0.014 | 20.50 ± 2.33 | 91 ± 24 | –127 ± 12 | 0.634 ± 0.109 | 0.754 ± 0.062 | 0.725 ± 0.054 |
| J0925+1409 | 0.164 ± 0.015 | 17.81 ± 3.26 | 81 ± 73 | –214 ± 151 | 0.652 ± 0.218 | 0.635 ± 0.094 | 0.638 ± 0.086 |
| J1152+3400 | 0.134 ± 0.022 | 20.94 ± 2.70 | 187 ± 48 | –468 ± 39 | 0.506 ± 0.067 | 0.619 ± 0.088 | 0.548 ± 0.053 |
| J1333+6246 | 0.151 ± 0.043 | 21.14 ± 1.46 | 102 ± 19 | –126 ± 48 | 0.731 ± 0.122 | 0.826 ± 0.066 | 0.804 ± 0.058 |
| J1442–0209 | 0.140 ± 0.015 | 19.60 ± 3.53 | 123 ± 183 | –261 ± 34 | 0.621 ± 0.120 | 0.549 ± 0.040 | 0.556 ± 0.038 |
| Tol1247–232 | 0.156 ± 0.010 | 21.89 ± 3.09 | 66 ± 87 | 260 ± 31 | 0.587 ± 0.061 | 0.690 ± 0.084 | 0.623 ± 0.049 |
| Tol0440–381 | 0.271 ± 0.028 | – | – | – | – | 0.570 ± 0.084 | 0.570 ± 0.084 |
| Mrk54 | 0.359 ± 0.013 | – | – | – | – | 0.504 ± 0.077 | 0.504 ± 0.077 |
| J0926+4427 | 0.114 ± 0.010 | 16.39 ± 0.40 | 213 ± 23 | –199 ± 12 | 0.723 ± 0.048 | 0.814 ± 0.048 | 0.768 ± 0.034 |
| J1429+0643 | 0.108 ± 0.015 | 16.17 ± 0.50 | 236 ± 56 | –241 ± 36 | 0.897 ± 0.071 | 0.960 ± 0.061 | 0.930 ± 0.046 |
| GP0303–0759 | 0.121 ± 0.045 | 16.07 ± 1.50 | 192 ± 99 | –266 ±92 | 0.908 ± 0.207 | – | 0.908 ± 0.207 |
| GP1244+0216 | 0.290 ± 0.043 | 16.34 ± 0.80 | 220 ± 79 | –78 ± 48 | 0.909 ± 0.357 | 0.950 ± 0.131 | 0.946 ± 0.123 |
| GP1054+5238 | 0.204 ± 0.044 | 19.60 ± 3.81 | 164 ± 78 | –166 ± 29 | 0.702 ± 0.131 | 0.889 ± 0.158 | 0.778 ± 0.101 |
| GP0911+1831 | 0.352 ± 0.038 | 16.76 ± 1.19 | 188 ± 43 | –273 ± 40 | 0.731 ± 0.150 | 0.765 ± 0.116 | 0.752 ± 0.092 |
| SGAS J1226 | 0.201 ± 0.001 | 17.16 ± 1.06 | 380 ± 24 | –264 ± 21 | 0.932 ± 0.038 | 0.998 ± 0.009 | 0.994 ± 0.009 |
| SGAS J1527 | 0.370 ± 0.002 | 17.15 ± 1.22 | 269 ± 47 | –208 ± 25 | 1.000 ± 0.075 | 0.990 ± 0.038 | 0.992 ± 0.034 |
| Cosmic Eye | 0.405 ± 0.001 | 22.59 ± 1.28 | 199 ± 5 | 56 ± 16 | 0.918 ± 0.072 | 0.998 ± 0.024 | 0.990 ± 0.023 |
Notes. Column 1: Galaxy name; Col. 2: dust attenuation parameter (EB-V); Col. 3: logarithm of the H I column density; Col. 4: H I Doppler b-parameter; Col. 5: H I velocity shift; and Col. 6: H I covering fraction from the fits. Uncertainties of the H I column density and covering fraction from the fits include the systematic errors detailed in Sect 4.2. Column 7: H I covering fraction measurements derived from the residual flux of the individual H I absorption lines (Sect. 3.3.1; Table C.3). GP0303–0759 does not have a reliable depth measurement because Milky Way absorption lines overlap the Lyman series; Col. 8: weighted mean of Cols. 6 and 7.
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