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Table A.5

Classification of the sample objects on the basis of the nuclear X-ray obscuration (and its variability).

Name ObsID Γ EW Fx/F[OIII] Ref.1 CT? Classification
(keV) [OIII]
(1) (2) (3) (4) (5) (6) (7) (8)

ESO 540-G01 0044350101 1.44 <0.48 Compton-thin
ESO 195-IG21 0554500201 1.29 0.11 Compton-thin
13898 2.06 0.51
ESO 113-G10 0103861601 1.62 <0.18 Compton-thin
0301890101 1.80 <0.04
NGC 526A 0109130201 1.30 0.08 75.4 1 Compton-thin
0150940101 1.55 0.06 99.4
0721730301 1.48 0.07 114.2
0721730401 1.58 0.06 137.3
342 <0.53 <0.23 19.4
MARK 609 0103861001 1.59 <0.16 31.1 2 Compton-thin
0402110201 1.25 0.11 32.5
NGC 1365 0151370101 1.18 0.20 13.2 1 Changing-look
0151370201 <1.36 <0.31 2.2
0151370701 2.44 0.14 17.0
0205590301 2.88 0.11 19.1
0205590401 2.18 0.17 14.5
0505140201 <0.39 0.46 3.9
0505140401 <0.09 0.42 7.1
0505140501 <0.17 0.43 5.6
0692840201 2.08 0.12 17.4
0692840301 2.40 0.09 18.2
0692840401 2.32 0.08 18.2
0692840501 2.20 0.09 17.8
6869 1.34 0.13 13.2
NGC 2617 0701981601 1.60 0.06 Compton-thin
0701981901 1.70 0.05
MARK 1218 0302260201 1.34 <0.09 18.1 2 Compton-thin
0302260401 1.670 <0.20 8.1
NGC 2992 0654910501 1.54 0.16 2.2 1 Changing-look
0654910601 1.31 0.33 0.9
0654910701 1.26 0.32 0.9
0654910901 1.23 0.50 0.5
0654911001 1.30 0.25 1.0
0701780101 1.39 0.17 2.8
POX52 0302420101 1.48 <0.11 8.2 3 Compton-thin
5736 1.79 <0.45 12.5
NGC 4138 0112551201 1.23 0.08 478.6 4 Compton-thin
3994 1.29 0.17 478.6
NGC 4395 0112521901 1.28 0.11 64.8 4 Compton-thin
5301 1.24 <0.11 27.7
5302 1.26 <0.10 25.8
NGC 4565 0112550301 1.55 <0.71 5.6 5 Compton-thin
3950 2.73 0.03 15.4
MARK 883 0302260101 1.22 <0.17 27.5 2 Compton-thin
0302260701 1.44 0.12 26.2
0302261001 1.58 0.10 32.3
0652550201 1.43 0.18 19.9
IRAS 20051-1117 0044350201 1.68 0.21 13.8 Compton-thin
0044350501 1.70 <0.16 9.5 5

Notes. (Column 1) name, (Col. 2) obsID, (Cols. 3 and 4) index of the power law and the equivalent width of the FeKα line from the spectral fit (PL model) in the 3–10 keV energy band, (Col. 5) ratio between the individual hard X-ray luminosity (from Table A.3) and the extinction-corrected [O III] fluxes, (Col. 6) references for the measure of F[OIII], (Col. 7) classification from the individual observation, (Col. 8) classification of the object, and (Col. 9) slope of the power law at hard energies for Compton-thick candidates from the simultaneous analysis (see Sect. 4.5).

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