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Table 2.
Dust extinction and H I properties derived from the Lyman series.
| Galaxy name | EB − V | Cf(H I) |
 |
 |
|---|---|---|---|---|
| [mag] | [km s−1] | [km s−1] | ||
| (1) | (2) | (3) | (4) | (5) |
| J1243+4646 | 0.100 ± 0.021 | < 0.189 | – | – |
| J1154+2443 | 0.118 ± 0.031 | 0.450 ± 0.086 | −289 ± 92 | 170 ± 86 |
| J1256+4509 | 0.076 ± 0.029 | 0.409 ± 0.079 | −48 ± 44 | 250 ± 50 |
| J1152+3400 ( * ) | 0.144 ± 0.021 | 0.625 ± 0.054 | −346 ± 28 | 419 ± 60 |
| J1442–0209 | 0.140 ± 0.015 | 0.556 ± 0.038 | −261 ± 34 | 371 ± 53 |
| J0925+1409 | 0.164 ± 0.015 | 0.638 ± 0.086 | −214 ± 151 | 320 ± 60 |
| J1011+1947 | 0.230 ± 0.084 | 0.708 ± 0.113 | −69 ± 32 | 285 ± 54 |
| J1503+3644 ( * ) | 0.217 ± 0.014 | 0.721 ± 0.055 | −79 ± 24 | 356 ± 49 |
| J1333+6246 | 0.151 ± 0.043 | 0.804 ± 0.058 | −126 ± 48 | 280 ± 51 |
| J0901+2119 | 0.220 ± 0.057 | 0.637 ± 0.166 | −121 ± 84 | 300 ± 78 |
| J1248+4259 | 0.253 ± 0.073 | 0.954 ± 0.104 | 56 ± 49 | 232 ± 50 |
| J0921+4509 | 0.222 ± 0.015 | 0.761 ± 0.080 | −56 ± 13 | 440 ± 20 |
| Tol1247–232 ( * ) | 0.195 ± 0.028 | 0.518 ± 0.046 | 194 ± 41 | 453 ± 89 |
| J0926+4427 ( * ) | 0.175 ± 0.010 | 0.768 ± 0.034 | −199 ± 12 | 383 ± 46 |
| J1429+0643 ( * ) | 0.165 ± 0.020 | 0.931 ± 0.046 | −220 ± 36 | 420 ± 50 |
| GP0303−0759 | 0.121 ± 0.045 | 0.908 ± 0.207 | −266 ± 92 | 380 ± 50 |
| GP1244+0216 | 0.290 ± 0.043 | 0.946 ± 0.123 | −78 ± 48 | 379 ± 49 |
| GP1054+5238 ( * ) | 0.253 ± 0.054 | 0.823 ± 0.101 | −161 ± 29 | 480 ± 29 |
| GP0911+1831 | 0.352 ± 0.038 | 0.752 ± 0.092 | −273 ± 40 | 374 ± 16 |
| SGAS J1226 | 0.201 ± 0.001 | 0.994 ± 0.009 | −264 ± 21 | 548 ± 29 |
| SGAS J1527 ( * ) | 0.314 ± 0.002 | 0.990 ± 0.034 | −247 ± 25 | 480 ± 30 |
| Cosmic Eye ( * ) | 0.371 ± 0.006 | 0.990 ± 0.023 | 311 ± 16 | 467 ± 99 |
Notes. (1) Galaxy name; (2) dust attenuation parameter ; (3) H I covering fraction; (4) H I velocity shift; (5) H I velocity width of maximal absorption. ( * )Changes with respect to Gazagnes et al. (2018), see Sect. 3 for details.
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