Table 1.
Properties of the galaxies in our sample.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
|---|---|---|---|---|---|---|---|---|
| Galaxy ID | z | log (M*/M⊙) | log (Mvir/M⊙) | rvir (kpc) | Tvir (106 K) | R (kpc) | ncl | log(NH/cm−2) |
| J094632.40+512335.9 | 0.41 | 11.2 | 13.0 | 427 | 3.3 | 42 | 5 | 19.5 |
| J140625.97+250923.2 | 0.40 | 11.1 | 12.9 | 397 | 2.8 | 47 | 5 | 19.2 |
| J111132.33+554712.8 | 0.46 | 11.4 | 13.4 | 564 | 6.3 | 77 | 3 | 19.2 |
| J080357.74+433309.9 | 0.25 | 11.1 | 12.9 | 433 | 2.6 | 78 | 4 | 18.6 |
| J092554.18+400353.4 | 0.25 | 11.1 | 12.9 | 435 | 2.6 | 84 | 1 | 19.9 |
| J095000.86+483102.2 | 0.21 | 11.0 | 12.7 | 381 | 1.9 | 94 | 4 | 19.7 |
| J112755.83+115438.3 | 0.42 | 11.2 | 12.9 | 423 | 3.3 | 99 | 2 | 17.7 |
| J124307.36+353926.3 | 0.39 | 11.3 | 13.2 | 504 | 4.4 | 102 | − | − |
| J155047.70+400122.6 | 0.31 | 11.2 | 13.0 | 452 | 3.1 | 107 | 4 | 18.9 |
| J024651.20-005914.1 | 0.41 | 11.4 | 13.4 | 581 | 6.1 | 109 | 6 | 19.2 |
| J135727.27+043603.3 | 0.33 | 11.3 | 13.2 | 522 | 4.3 | 126 | 1 | 19.0 |
| J091027.70+101357.2 | 0.26 | 11.2 | 13.0 | 465 | 3.1 | 140 | 4 | 18.5 |
| J141307.39+091956.7 | 0.36 | 11.7 | 14.1 | 1028 | 17.6 | 149 | − | − |
| J155304.32+354853.9 | 0.47 | 11.0 | 12.6 | 326 | 2.1 | 156 | 2 | 17.8 |
| J125859.98+413128.2 | 0.28 | 11.6 | 13.8 | 855 | 10.7 | 159 | − | − |
| J124409.17+172111.9 | 0.56 | 11.5 | 13.5 | 623 | 8.9 | 160 | 3 | 18.2 |
Notes. (1) galaxy name; (2) galaxy redshift; (3) galaxy stellar mass; (4) galaxy virial mass, calculated using the relation of Kravtsov et al. (2018) as explained in Sect. 2; (5) virial radius, see Sect. 2; (6) virial temperature (Eq. (2)); (7) projected distance between the line of sight and the galaxy; (8) number of observed clouds; (9) total hydrogen column density. All the data are taken from Chen et al. (2018), and Zahedy et al. (2019).
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