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Table 2.

Results of the X-ray spectral analysis and derived quantities.

Source HR Γ C/ν NH(z) ΔC F2 − 10 keV log L2 keV αox Δαox
J0303−00 1.87 553/608 < 1.2 0.0 3.61 27.59 −1.68 +0.02
J0304−00 1.99 596/660 1.1 −2.5 4.55 27.75 −1.64 +0.07
J0826+31 1.56 186/213 < 0.9 0.0 1.44 27.03 −1.87 −0.17
J0835+21 1.77 569/676 < 0.3 0.0 3.97 27.55 −1.67 +0.03
J0900+42 1.83 868/1034 < 0.1 0.0 17.09 28.27 −1.56 +0.20
J0901+35 1.60 527/563 0.6 −0.5 2.14 27.22 −1.82 −0.12
J0905+30 2.12 668/710 < 0.3 0.0 5.14 27.76 −1.60 +0.11
J0942+04 2.11 385/417 < 1.6 0.0 3.39 27.66 −1.70 +0.02
J0945+23 < −0.13 1.8(f) 109/123 14 −1.4 < 0.44 < 26.65 −1.97 −0.30
J0947+14 1.88 643/680 1.1 −3.2 4.90 27.66 −1.71 +0.03
J1014+43 2.21 395/479 < 0.3 0.0 3.19 27.61 −1.83 −0.05
J1027+35 1.91 632/683 < 0.2 0.0 7.08 27.86 −1.71 +0.05
J1111−15 1.71 326/394 < 0.8 0.0 1.00 26.91 −1.88 −0.20
J1111+24 1.77 376/383 < 0.3 0.0 1.33 27.10 −1.91 −0.19
J1143+34 1.94 674/734 < 0.1 0.0 4.52 27.69 −1.68 +0.04
J1148+23 1.16 338/317 < 1.6 0.0 1.21 26.79 −2.12 −0.35
J1159+31 1.8(f) 186/163 < 9.3 0.0 < 0.34 < 26.46 −2.14 −0.42
J1201+01 1.60 320/348 4.0 −3.0 0.71 26.78 −2.00 −0.30
J1220+45 1.70 221/240 < 5.7 0.0 0.47 26.66 −2.04 −0.34
J1225+48 1.89 813/882 < 0.2 0.0 6.70 27.82 −1.59 +0.12
J1246+26 2.00 458/565 0.9 −1.2 2.56 27.44 −1.75 −0.04
J1246+11 2.14 449/504 < 0.8 0.0 1.97 27.39 −1.70 −0.02
J1407+64 2.07 482/555 < 0.3 0.0 3.89 27.65 −1.71 +0.02
J1425+54 > 0.31 1.8(f) 182/182 10 −2.8 < 0.74 < 26.88 −1.99 −0.28
J1426+60 1.81 685/795 < 0.5 0.0 8.03 27.90 −1.74 +0.04
J1459+00 1.72 199/204 3.0 −0.7 1.21 26.99 −1.91 −0.20
J1507+24 1.8(f) 92/121 < 2.3 0.0 < 0.24 < 26.30 −1.96 −0.34
J1532+37 1.69 336/407 < 1.5 0.0 1.59 27.12 −1.92 −0.18
J1712+57 1.68 663/794 0.9 −2.7 7.54 27.76 −1.62 +0.09
J2234+00 1.86 646/694 < 0.2 0.0 5.49 27.70 −1.68 +0.05

Notes. Columns: (1) source ID; (2) hardness ratio relative to the 0.5−2 keV (soft) and 2−8 keV (hard) bands, based on EPIC/pn events only and computed following the Bayesian estimation method of Park et al. (2006); (3) photon index of the continuum in the unabsorbed (baseline) model, phabs × zpowerlw, where (f) means that the parameter is frozen; (4) best-fit statistics of the baseline model; (5) column density local to the source in the absorbed model, phabs × zphabs × zpowerlw; (6) statistical improvement after allowing for local absorption, whose inclusion is always less significant than the (nominal) 95% level; (7) intrinsic rest-frame 2−10 keV flux/upper limit as inferred from the baseline/absorbed model, in 10−14 erg s−1 cm−2; (8) intrinsic monochromatic luminosity at rest-frame 2 keV, in erg s−1 Hz−1; (9) two-point UV (2500 Å) to X-ray (2 keV) spectral index; (10) deviation of αox from the LX/LUV relation of Risaliti & Lusso (2019). Typical statistical uncertainties on αox and Δαox are 0.02 and 0.04, respectively. Entries in italics are upper limits.

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