Table B.1.
Measurement of H I covering fraction derived from the fits and from the residual flux of the individual Lyman series.
| Galaxy name | Lyβ | Lyγ | Lyδ | Ly5 | Depth | Fits | Final |
|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| J1243+4646 | – | 0.200 ± 0.121 | 0.020 ± 0.120 | 0.140 ± 0.120 | 0.120 ± 0.069 | − | < 0.189 |
| J1154+2443 | − | 0.471 ± 0.128 | − | 0.474 ± 0.184 | 0.472 ± 0.105 | 0.404 ± 0.152 | 0.450 ± 0.086 |
| J1256+4509 | 0.369 ± 0.290 | − | 0.530 ± 0.165 | 0.329 ± 0.143 | 0.410 ± 0.101 | 0.407 ± 0.125 | 0.409 ± 0.079 |
| J1152+3400 | 0.619 ± 0.088 | − | − | − | 0.619 ± 0.088 | 0.629 ± 0.069 | 0.625 ± 0.054 |
| J1442−0209 | 0.589 ± 0.049 | 0.471 ± 0.068 | − | – | 0.549 ± 0.040 | 0.621 ± 0.120 | 0.556 ± 0.038 |
| J0925+1409 | 0.635 ± 0.094 | − | − | − | 0.635 ± 0.094 | 0.652 ± 0.218 | 0.638 ± 0.086 |
| J1011+1947 | 0.693 ± 0.376 | 0.616 ± 0.244 | − | 0.820 ± 0.210 | 0.727 ± 0.147 | 0.644 ± 0.265 | 0.708 ± 0.113 |
| J1503+3644 | 0.847 ± 0.157 | 0.723 ± 0.129 | 0.741 ± 0.112 | 0.744 ± 0.113 | 0.754 ± 0.062 | 0.611 ± 0.110 | 0.721 ± 0.055 |
| J1333+6246 | 0.773 ± 0.152 | 0.870 ± 0.103 | 0.804 ± 0.106 | − | 0.826 ± 0.066 | 0.731 ± 0.122 | 0.804 ± 0.058 |
| J0901+2119 | 0.590 ± 0.461 | 0.742 ± 0.247 | − | − | 0.708 ± 0.218 | 0.539 ± 0.257 | 0.637 ± 0.166 |
| J1248+4259 | − | 1.000 ± 0.170 | − | 0.903 ± 0.157 | 0.948 ± 0.115 | 0.980 ± 0.241 | 0.954 ± 0.104 |
| J0921+4509 | 0.769 ± 0.116 | − | − | − | 0.769 ± 0.116 | 0.754 ± 0.111 | 0.761 ± 0.080 |
| Tol1247-232 | 0.543 ± 0.135 | − | 0.644 ± 0.115 | 0.414 ± 0.175 | 0.564 ± 0.078 | 0.486 ± 0.061 | 0.518 ± 0.046 |
| J0926+4427 | 0.817 ± 0.057 | 0.807 ± 0.087 | – | − | 0.814 ± 0.048 | 0.673 ± 0.040 | 0.731 ± 0.031 |
| J1429+0643 | 0.955 ± 0.061 | − | − | − | 0.955 ± 0.061 | 0.898 ± 0.071 | 0.931 ± 0.046 |
| GP0303−0759 | − | − | − | − | − | 0.908 ± 0.207 | 0.908 ± 0.207 |
| GP1244+0216 | 0.985 ± 0.211 | 0.894 ± 0.204 | 1.000 ± 0.292 | − | 0.950 ± 0.131 | 0.909 ± 0.357 | 0.946 ± 0.123 |
| GP1054+5238 | 0.936 ± 0.318 | − | 0.891 ± 0.203 | 0.798 ± 0.420 | 0.889 ± 0.158 | 0.778 ± 0.131 | 0.823 ± 0.101 |
| GP0911+1831 | 0.718 ± 0.361 | 0.781 ± 0.189 | 0.825 ± 0.198 | 0.635 ± 0.282 | 0.765 ± 0.116 | 0.731 ± 0.150 | 0.752 ± 0.092 |
| SGAS J1226 | 1.000 ± 0.010 | 1.000 ± 0.030 | 0.981 ± 0.057 | 0.940 ± 0.060 | 0.998 ± 0.009 | 0.932 ± 0.038 | 0.994 ± 0.009 |
| SGAS J1527 | 0.858 ± 0.141 | 1.000 ± 0.045 | 1.000 ± 0.087 | 1.000 ± 0.201 | 0.990 ± 0.038 | 0.993 ± 0.078 | 0.990 ± 0.034 |
| Cosmic Eye | 1.000 ± 0.043 | 1.000 ± 0.063 | 1.000 ± 0.033 | 0.899 ± 0.166 | 0.998 ± 0.024 | 0.920 ± 0.070 | 0.990 ± 0.023 |
Notes. See Sect. 3.1. (1) Galaxy name; (2)–(5) residual flux of the individual Lyman series (from Lyβ to Ly5); (6) H I covering fraction from the residual flux of the individual Lyman series derived as the weighted average of the Cols. (2)–(5). Dashes indicate that these transitions were not observed/included owing to Milky Way absorption, geocoronal emission, or low S/N. (7) H I covering fraction obtained from the fitting method. (8) H I covering fraction of the galaxy, derived as the weighted average of the Cols. (6) and (7).
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