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Table 2.

Summary of fitted and computed quantities.

Source Rsub RFe Kα υFWHM Rrep RIA m Pvar Pvar tlc
(pc) (pc) (km s−1) (pc) (pc) F2−10 keV FFe Kα (years)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)
1H0707-495 ... ... ... > 0.00084 < 2083 −0.28 ± 0.27 1 0.37 0.1 ± 0.05 18.98
2MASXJ23444 5.85 ± 3.04 ... ... < 27579 1.42 ± 0.62 1 0.91 0.04 ± 0.04 6.36
3C120 0.49 ± 0.25 0.083 ± 0.053 1954 ± 625 < 1711 −0.13 ± 0.87 1 0.99 0.09 ± 0.05 13.37
3C273 4.11 ± 2.14 0.54 ± 1.24 2700 ± 3082 < 7096 0.43 ± 0.67 1 1 0.08 ± 0.03 18.07
3C445 0.71 ± 0.37 0.057 ± 0.026 4990 ± 1133 < 2820 1 0.53 0.07 ± 0.06 9.68
4C+29.30 0.36 ± 0.19 ... ... < 3229 1 0.47 0.1 ± 0.07 8.89
4C+74.26 1.29 ± 0.67 ... ... < 4789 1 0.99 0.04 ± 0.03 4.31
Cen A 0.04 ± 0.02 0.10 ± 0.05 1816 ± 461 < 0.039 < 157 1.14 ± 0.20 1 1 0.08 ± 0.03 18.03
Circinus Galaxy 0.08 ± 0.04 0.0050 ± 0.0004 1463 ± 69 < 0.15 95 ± 15 0.32 ± 0.18 1 1 0.11 ± 0.05 18.27
CygnusA 0.76 ± 0.40 ... ... 1.12 ± 0.72 1 1 0.05 ± 0.03 17.01
H1821+643 3.09 ± 1.61 ... ... < 8559 2.32 ± 0.76 1 1 0.06 ± 0.04 7.27
IC4329A 0.42 ± 0.22 0.16 ± 0.17 1503 ± 799 < 0.08 < 849 1.09 ± 0.28 1 1 0.1 ± 0.05 17.05
M81 0.00 ± 0.00 0.26 ± 0.63 1323 ± 1587 < 6 0.78 ± 0.34 1 1 0.05 ± 0.03 16.87
MCG-6-30-15 0.11 ± 0.06 ... ... < 0.00084 < 414 0.40 ± 0.58 1 1 0.1 ± 0.05 12.57
MR2251-178 0.98 ± 0.51 0.16 ± 0.19 2401 ± 1442 < 8.39 ⋅ 10−6 < 3196 0.17 ± 0.73 1 1 0.06 ± 0.04 15.04
MRK 1040 0.24 ± 0.13 ... ... < 878 0.83 ± 0.56 1 1 0.1 ± 0.07 13.07
MRK 1210 0.18 ± 0.09 0.023 ± 0.017 3666 ± 1291 < 8.39 ⋅ 10−5 < 712 0.67 ± 1.35 1 0.46 0.14 ± 0.11 6.84
MRK 273 0.15 ± 0.08 ... ... > 0.0059 < 1948 −0.76 ± 1.13 1 0.77 0.05 ± 0.03 2.85
MRK 290 0.19 ± 0.10 0.0040 ± 0.0045 4973 ± 2526 4.2 < 1539 0.32 ± 0.34 1 1 0.09 ± 0.07 15.10
MRK 3 0.33 ± 0.17 0.0040 ± 0.0009 2739 ± 321 < 0.84 < 717 1 1 0.11 ± 0.05 16.85
MRK 509 0.54 ± 0.28 0.054 ± 0.021 3442 ± 661 0.02 < 1780 0.39 ± 0.23 1 0.70 0.04 ± 0.03 11.88
MRK 766 0.11 ± 0.06 ... ... > 0.016 < 686 0.17 ± 0.24 1 0.96 0.1 ± 0.05 14.17
NGC 1068 0.12 ± 0.06 0.0050 ± 0.0014 3217 ± 491 < 0.318 795 ± 176 0.77 ± 0.24 1 1 0.09 ± 0.04 14.53
NGC 1275 0.47 ± 0.24 0.019 ± 0.031 3237 ± 2613 0.003 0.07 ± 0.31 1 1 0.1 ± 0.04 18.22
NGC 1365 0.07 ± 0.03 0.028 ± 0.017 3745 ± 1111 < 289 0.34 ± 0.06 1 1 0.08 ± 0.04 9.08
NGC 2992 0.05 ± 0.02 0.310 ± 0.209 1990 ± 672 < 412 0.24 ± 0.06 1 1 0.07 ± 0.05 9.99
NGC 3393 0.10 ± 0.05 0.009 ± 0.005 4572 ± 1343 < 664 1 1 0.1 ± 0.07 8.77
NGC 3516 0.11 ± 0.06 0.009 ± 0.003 3861 ± 598 < 471 0.11 ± 0.26 1 0.31 0.09 ± 0.08 6.04
NGC 3783 0.24 ± 0.13 0.029 ± 0.006 2146 ± 238 0.078 < 518 −0.18 ± 0.28 1 1 0.11 ± 0.05 16.93
NGC 4051 0.02 ± 0.01 0.0010 ± 0.0003 2984 ± 573 < 124 0.10 ± 0.07 1 1 0.11 ± 0.04 16.07
NGC 4151 0.07 ± 0.03 0.034 ± 0.008 2487 ± 279 1.26 < 178 0.15 ± 0.09 1 1 0.06 ± 0.03 15.81
NGC 4388 0.16 ± 0.08 0.0050 ± 0.0018 3070 ± 528 < 449 1 1 0.12 ± 0.08 8.95
NGC 5548 0.19 ± 0.10 0.028 ± 0.011 3257 ± 682 > 0.57 < 907 0.07 ± 0.11 1 0.94 0.08 ± 0.05 15.96
NGC 6300 0.03 ± 0.02 ... ... < 0.0008 < 161 1 0.54 0.10 ± 0.08 8.29
NGC 7469 0.20 ± 0.10 0.0040 ± 0.0034 3431 ± 1298 > 0.0008 < 862 −0.13 ± 0.32 1 0.72 0.11 ± 0.06 15.01
NGC 7582 0.27 ± 0.14 ... ... < 281 1 1 0.08 ± 0.05 17.6
PKS2153-69 0.16 ± 0.09 ... ... < 1470 1 0.43 0.10 ± 0.06 13
PictorA 0.26 ± 0.14 ... ... < 1813 0.63 ± 0.40 1 0.61 0.11 ± 0.05 14.99

Notes. Col. (1): Object name; Col. (2): Dust sublimation radius computed with equation 3 for the sources with a RFe Kα measurement; Col. (3): Fe Kα radius estimated from υFWHM; Col. (4): deconvolved full width at half maximum velocity; Col. (5) Size of the Fe Kα reprocessor computed in Sect. 4.2 with 1-σ errors or 2-σ limits; Col. (6) spatial extent of Fe Kα emitting region obtained from imaging analysis, where values denote largest bin with a 3-σ detection and with errors correspond to 25% of bin width, while upper limits are calculated for 25 (4″ for Cen A and 2MASXJ23444), below which the effects of pileup severely limit any estimate for this sample (see Sect. 5); Col. (7) FFe KαF2−10 keV slope and 1-σ errors; Col. (8) variability probability Pvar for continuum light curve; Col. (9) variability probability Pvar for Fe Kα line light curve; Cols. (10–12): 50% percentile of the distributions of normalized excess variance, , calculated through the Monte Carlo method described in Sect. 4.1.2, for the continuum and Fe Kα line light curves, as well as the ratio between them, for all AGN in the sample. Error bars represent the ∼1σ uncertainties due to different realizations of the observational Poisson noise in the light curves. Negative values can occur when the Poisson noise uncertainty is larger than the intrinsic variance in Eq. (5). Column (13): normalized excess variance of the simulated continuum light curve and ∼1σ uncertainties (see Sect. 4.2); Col. (14): maximum light curve timespan in years. Asymmetric upper and lower errors are calculated separately following Sect. 1.73 of Lyons (1991).

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