Open Access

Table B.2.

WISSH QSOs with 5 − 20 X-ray net (i.e. background-subtracted) counts.

WISSH ID SDSS ID z NH, gal HR NH Log(L2 − 10) Log(F0.5 − 10)
(1) (2) (3) (4) (5) (6) (7) (8)
WISSH01 J0045+1438 1.9897 5.50 −0.16 ± 0.30 15 . 0 13.0 + 15.0 $ 15.0_{-13.0}^{+15.0} $ 44.31 ± 0.27 −13.91 ± 0.11
WISSH02 J0124+0044 3.822 3.13 0 . 72 0.27 + 0.07 $ -0.72_{-0.27}^{+0.07} $ ≤0.1 45.42 ± 0.12 −13.43 ± 0.12
WISSH03 J0125−1027 3.3588 3.20 0 . 25 0.24 + 0.31 $ 0.25_{-0.24}^{+0.31} $ 50 . 0 35.0 + 50.0 $ 50.0_{-35.0}^{+50.0} $ 45.43 ± 0.14 −13.30 ± 0.11
WISSH16 J0941+3257 3.454 1.44 0 . 30 0.44 + 0.28 $ -0.30_{-0.44}^{+0.28} $ ≤16.5 45.14 ± 0.15 −13.59 ± 0.15
WISSH19 J0958+2827 3.434 1.46 −0.06 ± 0.24 ≤99.0 44.63 ± 0.07 −14.10 ± 0.07
WISSH21 J1013+5615 3.6507 0.91 0.00 ± 0.38 ≤132.0 45.20 ± 0.15 −13.59 ± 0.15
WISSH23 J1015+0020 4.407 2.90 0 . 16 0.22 + 0.10 $ -0.16_{-0.22}^{+0.10} $ ≤49.5 45.52 ± 0.10 −13.47 ± 0.10
WISSH29 J1051+3107 4.2742 2.12 0 . 63 0.30 + 0.10 $ -0.63_{-0.30}^{+0.10} $ ≤0.1 44.96 ± 0.18 −13.99 ± 0.18
WISSH34 J1110+1930 2.502 1.73 0 . 07 0.26 + 0.27 $ 0.07_{-0.26}^{+0.27} $ ≤82.5 45.14 ± 0.10 −13.25 ± 0.10
WISSH42 J1200+3126 2.9947 1.49 −0.53 ± 0.23 ≤24.8 45.55 ± 0.09 −13.04 ± 0.09
WISSH44 J1201+1206 3.512 1.89 0 . 35 0.26 + 0.19 $ -0.35_{-0.26}^{+0.19} $ ≤66.0 45.64 ± 0.10 −13.11 ± 0.10
WISSH51 J1237+0647 2.7891 1.53 −0.01 ± 0.28 ≤82.5 45.22 ± 0.11 −13.29 ± 0.11
WISSH52 J1245+0105 2.8068 1.42 0 . 18 0.32 + 0.27 $ -0.18_{-0.32}^{+0.27} $ 30 . 0 23.0 + 30.0 $ 30.0_{-23.0}^{+30.0} $ 44.82 ± 0.27 −13.75 ± 0.12
WISSH56 J1305+0521 4.101 1.88 0 . 06 0.26 + 0.24 $ -0.06_{-0.26}^{+0.24} $ ≤82.5 45.37 ± 0.09 −13.54 ± 0.09
WISSH79 J1633+3629 3.5747 1.14 0 . 14 0.38 + 0.31 $ -0.14_{-0.38}^{+0.31} $ ≤66.0 45.23 ± 0.15 −13.54 ± 0.15
WISSH80 J1639+2824 3.846 2.93 0.00 ± 0.38 70 . 0 55.0 + 80.0 $ 70.0_{-55.0}^{+80.0} $ 45.61 ± 0.33 −13.28 ± 0.15

Notes. Columns: (1) WISSH ID; (2) SDSS ID; (3) Redshift (from Saccheo et al. 2023); (4) Galactic column density (in units of 1020 cm−2); (5) Hardness Ratio; (6) Intrinsic column density (in units of 1022 cm−2); (7) Intrinsic 2 − 10 keV luminosity (in units of Log(L2 − 10/erg s−1)); (8) Observed 0.5 − 10 keV flux (in units of Log(F0.5 − 10/erg s−1 cm−2)).

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