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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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