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Table A.2.

X-ray spectral parameters for the sample.

No. Galaxy ΓH NH T1 T2 NH
(1) (2) (3) (4) (5)
45 UGC 08387
47 CGCG 436−030
49 NGC 0695
50 CGCG 043−099 2.0
51 MCG+07−23−019
52 NGC 6670 (E) 2.0
52 NGC 6670 (W)
53 UGC 02369 (S) 2.0
54 NGC 1614
56 NGC 5331 (N) −a −a −a
56 NGC 5331 (S)
57 IRAS F06076−2139(N) 2.0
57 IRAS F06076−2139(S) −d −d −d −d
60 IC 2810(NW) 2.0
60 IC 2810 (SE) 2.0 −b −b
63 IRAS 18090+0130 (E)
63 IRAS 18090+0130(W) −d −d −d −d
64 III Zw 035 (N) 2.0
65 NGC 3256
67 IRAS F16399−0937(N)
67 IRAS F16399−0937(S) −a −a −a
68 IRAS F16164−0746
69 IC 4687
69 IC 4686 2.0
69 IC 4689 2.0 −b −b
71 NGC 2623
72 IC 5298 1.8
73 IRAS 20351+2521
75 NGC 6090 (NE)
75 NGC6090 (SW) 2.0
79 NGC 5256 (NE) 1.8
79 NGC 5256 (SW)
80 IRAS F03359+1523(E) 2.0
81 ESO 550−IG025 (N) 2.0
81 ESO 550−IG025 (S) −a −a −a
82 NGC 0034 1.8
83 MCG+12−02−001 (E)
83 MCG+12−02−001 (W) −a −a −a
85 IRAS F17138−1017
95 ESO 440−IG058 (N) −c 3.91 −c −c
95 ESO 440−IG058 (S) 2.0
100 NGC 7130 1.8
104 NGC 7771
104 NGC 7770 2.0
105 NGC 7592 (E) 2.0
105 NGC 7592 (W)
106 NGC 6285 2.0 −b −b
106 NGC 6286 2.0
107 NGC 4922 (N) 1.8
110 NGC 3110
114 NGC 0232
117 MCG+08−18−013(E)
120 CGCG 049−057 −a −a −a
121 NGC 1068
123 UGC 02238 −a −a −a
127 MCG−03−34−064 1.8
134 ESO 350−IG038
136 MCG−01−60−022 1.8
141 IC 0564
141 IC 0563
142 NGC 5135 2.0
144 IC 0860 −d −d −d −d
147 IC 5179
148 CGCG 465−012
157 MCG−02−33−098 2.0
157 MCG−02−33−099 2.0
163 NGC 4418 −a −a −a
169 ESO 343−IG013 (N) −a −a −a
169 ESO 343−IG013 (S) −a −a −a
170 NGC 2146
174 NGC 5653
178 NGC 4194
179 NGC 7591 −d −d −d −d
182 NGC 0023
188 NGC 7552
191 ESO 420−G013
194 ESO 432−IG006 (NE) 1.8
194 ESO 432−IG006 (SW) 1.8
195 NGC 1961
196 NGC 7753 −c −c −c
196 NGC 7752 2.0
198 NGC 1365 1.8
199 NGC 3221
201 NGC 0838

Notes. Column (1): Spectral power-law slope in the 2−7 keV range. Column (2): Obscuring column density for galaxies with an absorbed AGN model fit in the 2−7 keV range, in units of 1023 cm−2. Column (3): external mekal model temperature. Column (4): Internal, absorbed mekal model temperature. Column (5): Obscuring column density associated with the internal mekal model, in units of 1022 cm−2.

(a)

Full spectrum fitted with a single power-law.

(b)

Soft band spectrum fitted with a single mekal component.

(c)

Full spectrum fitted with a single mekal component.

(d)

No fit. Values without errors are imposed, as described in Sect. 4.4.2. Errors reported correspond to 1σ for one parameter of interest, leaving 5 parameters free.

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