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Table 2.

Chandra observation log for the objects in the CGII sample.

No. Galaxy Obs ID Date Mode Exp. Time (ks) 0.5−7.0 keVa (cts) NH, Galb (1020 cm−2)
45 UGC 08387 7811 2007−02−19 VFAINT 14.07 277.9 ± 17.1 1.0
47 CGCG 436−030 15047 2012−11−24 VFAINT 13.82 168.6 ± 13.8 3.4
49 NGC 0695 15046 2013−01−01 VFAINT 14.78 312.9 ± 18.5 6.9
50 CGCG 043−099 15048 2012−11−23 VFAINT 14.78 71.9 ± 8.1 1.9
51 MCG+07−23−019 12977 2011−02−07 VFAINT 52.34 506.9 ± 26.8 1.0
52 NGC 6670 15049 2013−02−08 VFAINT 14.77 252.7 ± 16.8 3.9
53 UGC 02369 4058 2002−12−14 FAINT 9.68 120.6 ± 12.0 7.9
54 NGC 1614 15050 2012−11−21 VFAINT 15.76 800.0 ± 28.9 6.3
56 NGC 5331 15051 2013−05−12 VFAINT 14.78 121.9 ± 12.4 2.0
57 IRAS F06076−2139 15052 2012−12−12 VFAINT 14.78 52.4 ± 8.2 7.6
60 IC 2810 15053 2013−10−27 VFAINT 14.78 93.2 ± 11.7 2.5
63 IRAS 18090+0130 15054 2013−02−10 VFAINT 14.77 98.9 ± 11.3 20.2
64 III Zw 035 6855 2006−02−24 FAINT 14.98 81.4 ± 9.0 4.8
65 NGC 3256 835 2000−01−05 FAINT 27.80 8117.2 ± 102.3 9.1
67 IRAS F16399−0937 15055 2013−06−30 VFAINT 14.87 161.9 ± 14.4 13.0
68 IRAS F16164−0746 15057 2013−01−19 VFAINT 14.78 99.2 ± 11.3 11.3
69 IC 4686/7 15056 2012−11−19 VFAINT 14.48 519.7 ± 23.8 11.5
71 NGC 2623 4059 2003−01−03 FAINT 19.79 171.0 ± 14.1 3.1
72 IC 5298 15059 2013−02−04 VFAINT 14.78 222.8 ± 16.0 5.7
73 IRAS 20351+2521 15058 2012−12−13 VFAINT 13.56 146.8 ± 14.0 13.1
75 NGC 6090 6859 2006−05−14 FAINT 14.79 347.5 ± 19.3 1.6
79 NGC 5256 2044 2001−11−02 FAINT 19.69 1451.2 ± 43.5 1.7
80 IRAS F03359+1523 6856 2005−12−17 FAINT 14.76 108.2 ± 11.4 13.8
81 ESO 550−IG025 15060 2012−11−24 VFAINT 14.78 72.2 ± 10.6 3.2
82 NGC 0034 15061 2013−06−05 VFAINT 14.78 329.0 ± 19.5 2.1
83 MCG+12−02−001 15062 2012−11−22 VFAINT 14.31 311.0 ± 19.3 22.0
85 IRAS F17138−1017 15063 2013−07−12 VFAINT 14.78 207−3 ± 15.4 17.0
95 ESO 440−IG058 15064 2013−03−20 VFAINT 14.78 187.0 ± 16.1 5.6
100 NGC 7130 2188 2001−10−23 FAINT 38.64 3327.1 ± 59.3 1.9
104 NGC 7771 10397 2009−05−22 VFAINT 16.71 904.6 ± 34.6 4.0
105 NGC 7592 6860 2006−10−15 FAINT 14.99 388.7 ± 21.9 3.8
106 NGC 6286 10566 2009−09−18 FAINT 14.00 544.8 ± 27.9 1.8
107 NGC 4922 15065 2013−11−02 VFAINT 14.86 202.9 ± 17.2 0.9
110 NGC 3110 15069 2013−02−02 VFAINT 14.87 396.3 ± 22.3 3.5
114 NGC 0232 15066 2013−01−04 VFAINT 14.78 193.5 ± 15.7 1.4
117 MCG+08−18−013 15067 2013−06−03 VFAINT 13.79 101.7 ± 11.1 1.7
120 CGCG 049−057 10399 2009−04−17 VFAINT 19.06 30.2 ± 7.6 2.6
121 NGC 1068 344 2000−02−21 FAINT 47.44 100828.1 ± 326.7 2.9
123 UGC 02238 15068 2012−12−02 VFAINT 14.87 132.1 ± 13.5 8.9
127 MCG−03−34−064 7373 2006−07−31 FAINT 7.09 1029.3 ± 32.9 5.0
134 ESO 350−IG038 8175 2006−10−28 VFAINT 54.00 1794.5 ± 45.8 2.4
136 MCG−01−60−022 10570 2009−08−13 FAINT 18.90 325.4 ± 21.7 3.6
141 IC 0563/4 15070 2013−01−19 VFAINT 14.96 252.5 ± 18.9 3.8
142 NGC 5135 2187 2001−09−04 FAINT 29.30 3975.9 ± 68.0 4.9
144 IC 0860 10400 2009−03−24 VFAINT 19.15 25.9 ± 7.2 1.0
147 IC 5179 10392 2009−06−21 VFAINT 11.96 555.5 ± 32.2 1.4
148 CGCG 465−012 15071 2012−12−17 VFAINT 14.87 134.0 ± 13.4 14.8
157 MCG−02−33−098/9 15072 2013−05−08 VFAINT 14.87 141.0 ± 12.4 3.7
163 NGC 4418 4060 2003−03−10 FAINT 19.81 59.6 ± 15.3 1.9
169 ESO 343−IG013 15073 2013−06−13 VFAINT 14.78 139.6 ± 13.9 2.8
170 NGC 2146 3135 2002−11−16 FAINT 10.02 2144.2 ± 50.4 7.1
174 NGC 5653 10396 2009−04−11 VFAINT 16.52 387.1 ± 22.8 1.3
178 NGC 4194 7071 2006−09−09 FAINT 35.50 2410.3 ± 51.4 1.5
179 NGC 7591 10264 2009−07−05 FAINT 4.88 26.3 ± 6.1 5.6
182 NGC 0023 10401 2008−10−27 VFAINT 19.45 753.1 ± 31.9 3.4
188 NGC 7552 7848 2007−03−31 FAINT 5.08 832.8 ± 30.2 1.2
191 ESO 420−G013 10393 2009−05−13 VFAINT 12.42 759.0 ± 29.2 2.1
194 ESO 432−IG006 15074 2013−06−24 VFAINT 16.05 280.7 ± 20.0 19.3
195 NGC 1961 10531 2009−05−08 VFAINT 32.83 723.3 ± 40.0 8.1
196 NGC 7752/3 10569 2009−08−30 FAINT 11.99 96.0 ± 12.7 5.4
198 NGC 1365 6869 2006−04−20 FAINT 15.54 4644.2 ± 72.7 1.3
199 NGC 3221 10398 2009−03−19 VFAINT 19.03 323.5 ± 28.3 1.9
201 NGC 0838 15667 2013−07−21 VFAINT 58.34 1996.0 ± 49.6 2.6

Notes.

(a)

The source counts are background corrected and measured in the 0.5−7.0 keV band. The counts from separate components in a single system are obtained separately and then summed together.

(b)

The Galactic absorption column density is taken from the LAB HI map by Kalberla et al. (2005).

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