Table 2.
Summary of fitted and computed quantities.
Source | Rsub | RFe Kα | υFWHM | Rrep | RIA | m | Pvar | Pvar | ![]() |
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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 |
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0.1 ± 0.05 | 18.98 |
2MASXJ23444 | 5.85 ± 3.04 | ... | ... | — | < 27579 | 1.42 ± 0.62 | 1 | 0.91 |
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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 |
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0.09 ± 0.05 | 13.37 |
3C273 | 4.11 ± 2.14 | 0.54 ± 1.24 | 2700 ± 3082 | — | < 7096 | 0.43 ± 0.67 | 1 | 1 |
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0.08 ± 0.03 | 18.07 |
3C445 | 0.71 ± 0.37 | 0.057 ± 0.026 | 4990 ± 1133 | — | < 2820 | — | 1 | 0.53 |
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0.07 ± 0.06 | 9.68 |
4C+29.30 | 0.36 ± 0.19 | ... | ... | — | < 3229 | — | 1 | 0.47 |
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0.1 ± 0.07 | 8.89 |
4C+74.26 | 1.29 ± 0.67 | ... | ... | — | < 4789 | — | 1 | 0.99 |
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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 |
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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 |
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0.11 ± 0.05 | 18.27 |
CygnusA | 0.76 ± 0.40 | ... | ... | — | — | 1.12 ± 0.72 | 1 | 1 |
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0.05 ± 0.03 | 17.01 |
H1821+643 | 3.09 ± 1.61 | ... | ... | — | < 8559 | 2.32 ± 0.76 | 1 | 1 |
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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 |
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0.1 ± 0.05 | 17.05 |
M81 | 0.00 ± 0.00 | 0.26 ± 0.63 | 1323 ± 1587 | — | < 6 | 0.78 ± 0.34 | 1 | 1 |
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0.05 ± 0.03 | 16.87 |
MCG-6-30-15 | 0.11 ± 0.06 | ... | ... | < 0.00084 | < 414 | 0.40 ± 0.58 | 1 | 1 |
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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 |
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0.06 ± 0.04 | 15.04 |
MRK 1040 | 0.24 ± 0.13 | ... | ... |
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< 878 | 0.83 ± 0.56 | 1 | 1 |
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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 |
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0.14 ± 0.11 | 6.84 |
MRK 273 | 0.15 ± 0.08 | ... | ... | > 0.0059 | < 1948 | −0.76 ± 1.13 | 1 | 0.77 |
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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 |
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0.09 ± 0.07 | 15.10 |
MRK 3 | 0.33 ± 0.17 | 0.0040 ± 0.0009 | 2739 ± 321 | < 0.84 | < 717 | — | 1 | 1 |
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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 |
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0.04 ± 0.03 | 11.88 |
MRK 766 | 0.11 ± 0.06 | ... | ... | > 0.016 | < 686 | 0.17 ± 0.24 | 1 | 0.96 |
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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 |
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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 |
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0.1 ± 0.04 | 18.22 |
NGC 1365 | 0.07 ± 0.03 | 0.028 ± 0.017 | 3745 ± 1111 |
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< 289 | 0.34 ± 0.06 | 1 | 1 |
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0.08 ± 0.04 | 9.08 |
NGC 2992 | 0.05 ± 0.02 | 0.310 ± 0.209 | 1990 ± 672 |
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< 412 | 0.24 ± 0.06 | 1 | 1 |
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0.07 ± 0.05 | 9.99 |
NGC 3393 | 0.10 ± 0.05 | 0.009 ± 0.005 | 4572 ± 1343 | — | < 664 | — | 1 | 1 |
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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 |
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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 |
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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 |
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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 |
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0.06 ± 0.03 | 15.81 |
NGC 4388 | 0.16 ± 0.08 | 0.0050 ± 0.0018 | 3070 ± 528 |
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< 449 | — | 1 | 1 |
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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 |
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0.08 ± 0.05 | 15.96 |
NGC 6300 | 0.03 ± 0.02 | ... | ... | < 0.0008 | < 161 | — | 1 | 0.54 |
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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 |
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0.11 ± 0.06 | 15.01 |
NGC 7582 | 0.27 ± 0.14 | ... | ... |
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< 281 | — | 1 | 1 |
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0.08 ± 0.05 | 17.6 |
PKS2153-69 | 0.16 ± 0.09 | ... | ... | — | < 1470 | — | 1 | 0.43 |
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0.10 ± 0.06 | 13 |
PictorA | 0.26 ± 0.14 | ... | ... | — | < 1813 | 0.63 ± 0.40 | 1 | 0.61 |
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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 Kα–F2−10 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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