Table 2
Results of the variability analysis.
| Name | Type | log (Lsoft) | log (Lhard) | log (MBH) | log (REdd) | Variability | ΔTmax | ||
|
|
|||||||||
| (0.5−2 keV) | (2−10 keV) | SMF0 | SMF1 | SMF2 | (Years) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
|
|
|||||||||
| MARK 348 (X) | HBLR | 42.76 | 43.15 | 7.58 | –1.02 | ME2PL | Nor m 2 | – | 10 |
69 5% |
683% |
69 % |
|||||||
| NGC 424 (C, X)* | HBLR | 41.74 | 41.85 | 7.78 | –2.53 | 2ME2PL | – | – | 0.16 |
| 0% | 0% | ||||||||
| MARK 573 (C)* | HBLR | 41.65 | 41.54 | 7.37 | –2.42 | 2ME2PL | – | – | 4 |
| 0% | 0% | (+3gauss) | |||||||
| (X, C) | 41.73 | 41.41 | 2ME2PL | – | – | 2 | |||
| 0% | 0% | ||||||||
| NGC 788 (X, C) | HBLR | 42.11 | 42.60 | 7.43 | –1.43 | 2ME2PL | – | – | 0.33 |
| 0% | 0% | ||||||||
| ESO 417-G06 (X) | – | 42.46 | 42.50 | 7.44 | –1.53 | MEPL | N H2 | – | 0.08 |
| 0% | 0% | 21 % |
|||||||
| MARK 1066 (X, C)* | NHBLR | 41.40 | 41.43 | 7.23 | –2.38 | ME2PL | – | – | 2 |
| 0% | 0% | ||||||||
| 3C 98.0 (X) | – | 43.13 | 42.80 | 7.75 | –1.73 | MEPL | Nor m 2 | – | 0.41 |
| 54% |
427% |
43 % |
|||||||
| (X, C) | 42.40 | 42.60 | MEPL | – | – | 5 | |||
| 0% | 0% | ||||||||
| MARK 3 (X)* | HBLR | 42.24 | 42.74 | 8.74 | –2.58 | 2ME2PL | Nor m 2 | – | 1 |
| 297% |
324% |
37 % |
|||||||
| MARK 1210 (C) | HBLR | 42.31 | 42.79 | 7.70 | –1.50 | 2ME2PL | Nor m 2 | N H2 | 4 |
| 75% |
71% |
11 % |
20 % |
||||||
| IC 2560 (X, C)* | – | 40.57 | 41.03 | 6.46 | –2.02 | 2ME2PL | – | – | 0.16 |
| 0% | 0% | (+1gauss) | |||||||
| NGC 3393 (C)* | – | 41.64 | 41.29 | 8.10 | –3.41 | 2ME2PL | – | – | 7 |
| 0% | 0% | ||||||||
| (X, C) | 41.44 | 41.26 | 2ME2PL | – | – | 0.66 | |||
| 0% | 0% | ||||||||
| NGC 4507 (X) | HBLR | 42.04 | 42.67 | 8.26 | –2.28 | 2ME2PL | Nor m 2 | N H2 | 9 |
| 964% |
8110% |
(+2gauss) | 51 % |
4 % |
|||||
| (X, C) | 41.96 | 42.85 | Nor m 2 | – | 0.41 | ||||
| 453% |
383% |
53 % |
|||||||
| NGC 4698 (X) | – | 40.14 | 40.08 | 7.53 | –4.04 | 2PL | – | – | 9 |
| 0% | 0% | ||||||||
| NGC 5194 (C)* | NHBLR | 39.53 | 39.51 | 6.73 | –3.82 | ME2PL | – | – | 11 |
| 0% | 0% | ||||||||
| (X, C) | 39.94 | 39.39 | 2ME2PL | – | – | 0.6 | |||
| 0% | 0% | ||||||||
| MARK 268 (X) | – | 41.34 | 42.92 | 7.95 | –1.62 | ME2PL | – | – | 0.01 |
| 0% | 0% | ||||||||
| MARK 273 (X, C)CL? | – | 41.34 | 42.29 | 7.74 | –2.05 | 2ME2PL | N H2 | – | 2 |
| 242% |
326% |
51 % |
|||||||
| Circinus (C)* | HBLR | 39.80 | 40.60 | 7.71 | –3.71 | 2ME2PL | – | – | 9 |
| 0% | 0% | (+4gauss) | |||||||
| NGC 5643 (X)* | NHBLR | 40.44 | 40.87 | 6.30 | –2.02 | 2ME2PL | – | – | 6 |
| 0% | 0% | ||||||||
| MARK 477 (X)* | HBLR | 42.60 | 43.11 | 7.20 | –0.68 | 2ME2PL | – | – | 0.01 |
| 0% | 0% | ||||||||
| IC 4518A (X) | – | 42.06 | 42.45 | 7.48 | –1.63 | 2ME2PL | Nor m 2 | – | 0.02 |
| 402% |
416% |
42 % |
|||||||
| ESO 138-G01 (X)* | – | 42.23 | 42.11 | 5.50 | 0.01 | ME2PL | – | – | 6 |
| 0% | 0% | ||||||||
| NGC 6300 (C) | – | 41.32 | 41.95 | 7.18 | –2.68 | 2PL | – | – | 0.01 |
| 0% | 0% | ||||||||
| (X, C) | 41.06 | 41.68 | 2PL | Nor m 2 | Nor m 1 | 8 | |||
| 9850% |
9816% |
98 % |
93 % |
||||||
| NGC 7172 (X) | NHBLR | 42.50 | 42.82 | 8.20 | –1.98 | ME2PL | Nor m 2 | – | 5 |
| 512% |
511% |
51% |
|||||||
| NGC 7212 (X, C)* | HBLR | 41.81 | 42.60 | 7.54 | –1.55 | 2ME2PL | – | – | 1 |
| 0% | 0% | ||||||||
| NGC 7319 (C)CL? | – | 42.99 | 42.98 | 7.43 | –1.26 | ME2PL | Nor m 2 | N H1 | 7 |
| 388% |
385% |
39 % |
100 % |
||||||
| (X, C) | 42.58 | 42.84 | ME2PL | Nor m 2 | – | 6 | |||
| 718% |
697% |
72 % |
|||||||
Notes. Column 1: name (the asterisks represent Compton–thick or changing look candidates), and the instrument (C: Chandra and/or X: XMM-Newton) in parenthesis; Col. 2: (non) hidden broad line region objects only in the cases where there are available observations; Cols. 3 and 4: logarithm of the soft (0.5–2 keV) and hard (2–10 keV) X-ray luminosities, where the mean was calculated for variable objects, and percentages in flux variations; Col. 5: black-hole mass on logarithmical scale, determined using the correlation between stellar velocity dispersion (from HyperLeda) and black-hole mass (Tremaine et al. 2002), or obtained from the literature otherwise (MARK 1210 and NGC 4507 from Nicastro et al. 2003; IC 4518A from Alonso-Herrero et al. 2013; NGC 6300 and NGC 5643 from Davis et al. 2014; IC 2560 from Baloković et al. 2014; MARK 268 from Khorunzhev et al. 2012; and MARK 477 from Singh et al. 2011); Col. 6: Eddington ratio, Lbol/ ! LEdd, calculated from Eracleous et al. (2010) using Lbol = 33L2−10 keV; Col. 7: best fit for SMF0; Col. 8: parameter varying in SMF1, with the percentage of variation; Col. 9: parameter varying in SMF2, with the percentage of variation; Col. 10: and the sampling timescale, corresponding to the difference between the first and the last observation. The percentages correspond to this ΔTmax.
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