The sample

(1) WISSH ID; (2) SDSS ID; (3) redshift; (4) BH mass from Hβ in LBT/LUCI and VLT/SINFONI follow-up programs, except for (a) M_BH from MgII or (b) CIV, from the SDSS Quasar catalog Shen et al. (2011); (5) Bolometric luminosity and (6) Eddington ration from Saccheo et al. (2023); (7) CIV velocity shift (Vietri et al. 2018); (8) OIII velocity shift (Bischetti et al. 2017); (9) UV Absorption line velocity for BAL (Bruni et al. 2019) and NAL (Misawa et al. 2007).

(1) WISSH ID; (2) Available exposure from Chandra (C) or XMM (X); (3) total observed counts; (4) photon index; (5) 0.3-10keV Flux; (6) 2-10 keV Luminosity; (7) α_OX ; (8) requested net and total exposure time.