Table B.2.
Measurement of H I velocity width of the individual Lyman series. See Sect. 3.1.
| Galaxy name |
 |
 |
 |
 |
 |
|---|---|---|---|---|---|
| [km s−1] | [km s−1] | [km s−1] | [km s−1] | [km s−1] | |
| (1) | (2) | (3) | (4) | (5) | (6) |
| J1243+4646 | – | − | − | − | − |
| J1154+2443 | − | 170 ± 100 | − | 170 ± 170 | 170 ± 86 |
| J1256+4509 | 270 ± 80 | − | 220 ± 90 | 280 ± 90 | 250 ± 50 |
| J1152+3400 | 420 ± 60 | − | − | − | 420 ± 60 |
| J1442−0209 | 490 ± 80 | 280 ± 70 | − | – | 371 ± 53 |
| J0925+1409 | 320 ± 60 | − | − | − | 320 ± 60 |
| J1011+1947 | 420 ± 80 | 170 ± 90 | − | 170 ± 130 | 285 ± 54 |
| J1503+3644 | 410 ± 90 | 380 ± 100 | 280 ± 100 | 340 ± 100 | 356 ± 49 |
| J1333+6246 | 320 ± 80 | 280 ± 100 | 230 ± 90 | − | 280 ± 51 |
| J0901+2119 | 320 ± 110 | 280 ± 110 | − | − | 300 ± 78 |
| J1248+4259 | − | 260 ± 90 | − | 220 ± 60 | 232 ± 50 |
| J0921+4509 | 440 ± 20 | − | − | − | 440 ± 20 |
| Tol1247−232 | 530 ± 140 | − | 360 ± 180 | 430 ± 150 | 453 ± 89 |
| J0926+4427 | 400 ± 60 | 360 ± 70 | – | − | 383 ± 46 |
| J1429+0643 | 420 ± 50 | − | − | − | 420 ± 50 |
| GP0303−0759 | 380 ± 50 | − | − | − | 380 ± 50 |
| GP1244+0216 | 380 ± 50 | 370 ± 205 | − | − | 379 ± 49 |
| GP1054+5238 | 580 ± 50 | − | 400 ± 50 | 460 ± 50 | 480 ± 29 |
| GP0911+1831 | 410 ± 60 | 410 ± 50 | 370 ± 20 | 350 ± 40 | 374 ± 16 |
| SGAS J1226 | 560 ± 40 | 600 ± 80 | – | 510 ± 50 | 548 ± 29 |
| SGAS J1527 | 610 ± 60 | 520 ± 70 | − | 410 ± 40 | 480 ± 30 |
| Cosmic Eye | 700 ± 380 | 740 ± 210 | 320 ± 140 | 450 ± 220 | 467 ± 99 |
Notes. (1) Galaxy name; (2)–(5) velocity width of the individual Lyman series (from Lyβ to Ly5); (6) H I velocity width 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, low S/N, or irregular line shape.
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