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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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