Table 7
Results for the best fit of the annular region (ring) in Chandra data, and the best fit obtained for the nucleus of XMM-Newton data when the contribution from the annular region was removed.
| Name (obs ID) | Region | Model | N H1 | N H2 | kT | Γ |
|
log Lsoft | log Lhard | Cont. |
| (1022 cm-2) | (1022 cm-2) | (keV) | (0.5–2 keV) | (2–10 keV) | % | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
|
|
||||||||||
| NGC 1052 (5910) | Ring | ME2PL | – |
|
|
|
1.47 | 40.185 | 40.563 | 10 |
| NGC 1052 (093630101) | Nucleus | ME2PL | – |
|
|
|
1.13 | 39.875 | 41.235 | |
|
|
||||||||||
| NGC 3226 (860) | Ring | PL | – | – | – |
|
1.89 | 40.482 | 40.557 | 20 |
| NGC 3226 (0101040301) | Nucleus | 2PL |
|
|
– |
|
1.00 | 40.623 | 40.912 | |
|
|
||||||||||
| NGC 3627 (9548) | Ring | MEPL | – | – |
|
|
1.35 | 39.302 | 39.384 | 92 |
| NGC 3627 (093641101) | Nucleus | MEPL | – | – |
|
|
1.16 | 38.990 | 38.125 | |
|
|
||||||||||
| NGC 4261 (9569) | Ring | MEPL |
|
|
|
|
2.07 | 40.663 | 40.252 | 37 |
| NGC 4261 (0502120101) | Nucleus | ME2PL | – |
|
|
|
1.21 | 40.857 | 41.051 | |
|
|
||||||||||
| NGC 4278 (7077) | Ring | MEPL | – | – |
|
|
1.12 | 39.551 | 39.707 | 38 |
| NGC 4278 (0205010101) | Nucleus | PL |
|
|
1.05 | 40.681 | 40.736 | |||
|
|
||||||||||
| NGC 4552 (2072) | Ring | MEPL | – | – |
|
|
1.47 | 39.648 | 39.304 | 23 |
| NGC 4552 (0141570101) | Nucleus | MEPL | – | – |
|
|
1.10 | 40.053 | 39.878 | |
|
|
||||||||||
| NGC 5846 (788) | Ring | MEPL | – | – |
|
|
1.63 | 40.815 | 40.217 | 73 |
| NGC 5846 (0021540101) | Nucleus | MEPL | – | – |
|
4.003.56 | 1.36 | 40.753 | 39.171 | |
Notes.Name and obs ID in parenthesis (Col. 1), extracted region (Col. 2), best-fit model (Col. 3), parameters of the best-fit model (Cols. 4–8), soft and hard intrinsic luminosities (Cols. 9 and 10), and the percentage of the contribution from the ring to the 25″ aperture Chandra data in the 0.5–10.0 keV band (Col. 11).
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