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Table B.1.

Best-fit results of sources with flux variabilities in our sample and M19 sample.

Source Csoft/NuS NH,los, NuS NH,los, soft ΔNH,los ΔT
2MASX J06411806+3249313 0.75 23.09 23.27 0.18 12.80
3C 105* 2.63 23.65 8.34
3C 445 1.43 23.08 23.21 0.13 14.44
3C 452 1.30 23.59 23.82 0.23 8.42
4C +29.30 1f 23.50 23.68 0.18 5.58
4C +73.08 1f 23.53 23.70 0.17 7.40
ESO 21-4* 1f 23.43 23.67 0.24 4.63
ESO 103-35 1.33 23.25 23.28 0.03 15.58
ESO 119-8* 2.01 23.17 0.03
ESO 263-13 0.81 23.85 23.43 0.42 1.67
ESO 383-18 1.43 23.28 23.32 0.04 10.03
ESO 439-G009 1f 23.58 23.69 0.11 0.54
ESO 553-43* 0.63 23.18 5.75
Fairall 272 0.83 23.23 23.51 0.27 6.24
IC 1657 3.11 23.53 8.20
IC 4518A 0.81 23.11 23.36 0.25 6.99
IC 4709 2.43 23.38 6.74
IRAS 16288+3929 1f 23.88 23.75 0.13 1.03
LEDA 259433 1f 23.05 23.34 0.29 1.54
LEDA 2816387* 1f 23.76 23.87 0.11 1.54
LEDA 511869 2.17 23.88 1.71
MCG -01-05-047 1.23 23.33 23.23 0.10 3.35
MCG +11-11-32 0.68 23.11 0.18
Mrk 348 0.93 22.92 23.14 0.22 13.28
Mrk 417 1f 23.53 23.81 0.28 10.68
Mrk 477 1f 23.30 23.70 0.40 3.82
Mrk 1210 1.30 23.30 11.42
NGC 454E 1f 23.86 23.37 0.49 6.27
NGC 612 1.49 23.95 6.22
NGC 788 1.59 23.79 3.04
NGC 835 1f 23.46 24.06 0.60 15.64
NGC 1142 1.43 24.20 23.75 0.45 11.71
NGC 3281 0.65 24.30 23.90 0.40 5.05
NGC 4388 1.89 23.43 5.70
NGC 4507 0.68 23.88 4.85
NGC 4939 1f 23.82 23.69 0.13 6.69
NGC 4941 1f 23.98 23.58 0.40 6.69
NGC 4992 1.12 23.46 23.67 0.21 10.58
NGC 5283 0.64 23.04 14.98
NGC 6300 0.085 23.21 23.34 0.13 15.48
NGC 7319 3.33 23.81 15.80
UGC 3995B 0.30 23.48 0.75
Z367-9 4.03 23.11 7.56
CGCG 164-19 1f 23.77 23.41 0.36 2.80
ESO 201-004 1f 24.34 24.19 0.15 7.07
NGC 7479 0.78 24.76 24.56 0.20 2.05
NGC 7582 0.56 24.23 23.58 0.65 3.66

Notes. Column 2: Cross-calibration factor between the soft X-ray spectra and NuSTAR spectra. Column 3: Logarithm of “line-of-sight” column density of NuSTAR observation in cm−2. Column 4: Logarithm of “line-of-sight” column density of soft X-ray observation in cm−2. Column 5: Absolute difference between NH,los, NuS and NH,los, soft. Column 6: Time interval between the NuSTAR observation and the soft X-ray observation in years. Sources labeled with asterisks are those fitted with only the line-of-sight component and the scattered component.

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