Table 11
Summary.
| Name | Type | log Lsoft | log Lhard | log MBH | Lbol/LEdd | Variability | T | HR | |||
| (0.5–2 keV) | (2–10 keV) | SMF0 | SMF1 | SMF2 | (Years) | ||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | |
|
|
|||||||||||
| NGC 1052 (X) | AGN | 41.04 | 41.52 | 8.07 | 7.2 × 10-4 | ME2PL | Nor m 2 | N H2 | 8 | ||
| 1.9 | 20% | 20% | 49% | 31% | 33% | ||||||
| NGC 3226 (X,C) | AGN | 40.78 | 41.01 | 8.22 | 1.6 × 10-4 | 2PL | N H2 | Nor m 2 | 1 | ||
| 1.9 | 37% | 81% | 93% | 57% | |||||||
| NGC 4261 (X) | AGN | 40.98 | 41.02 | 8.96 | 2.9 × 10-5 | ME2PL | – | – | 8 | ||
| 2 | 0% | 0% | 0% | ||||||||
| (C) | ME2PL | – | – | 6 | |||||||
| 0% | 0% | 19% | |||||||||
| NGC 4278 (C) | AGN | 39.80 | 39.75 | 8.46 | 5.0 × 10-6 | MEPL | Nor m 2 | – | 1 | ||
| 1.9 | 26% | 29% | 30% | 40%* | |||||||
| NGC 4552 (X,C) | AGN | 39.49 | 39.45 | 8.84 | 1.0 × 10-6 | MEPL | Nor m 1 | Nor m 2 | 2 | ||
| 2 | 73% | 63% | 93% | 78% | |||||||
| NGC 5846 (X) | Non-AGN | 40.29 | 39.33 | 8.49 | 1.8 × 10-6 | MEPL | – | – | 7 | ||
| 2 | 0% | 0% | 1% | ||||||||
| (C) | MEPL | – | – | 0.6 | |||||||
| 0% | 0% | 6% | |||||||||
Notes.Name, and the instrument in parenthesis (Col. 1), type (Col. 2), logarithm of the soft (0.5–2 keV) and hard (2–10 keV) X-ray luminosities, where the mean was calculated or Chandra luminosity was given when both instruments were used, and percentages in flux variations (Cols. 3 and 4), black-hole mass in logarithmical scale, from González-Martín et al. (2009a) (Col. 5), Eddington ratio, calculated from Eracleous (2010) using Lbol = 33 L2−10 keV (Col. 6), best fit for the SMF0 (Col. 7), parameter varying in SMF1, with the percentage of variation (Col. 8), parameter varying in SMF2, with the percentage of variation (Col. 9), the sampling timescale for variations (Col. 10), and variations in the hardness ratios (Col. 11).
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