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Table A.2.
Results of the X-ray spectral analysis with the baseline model.
| Parameters | NGC 2960 | NGC 6264 | NGC 6323 | UGC 3789 |
|---|---|---|---|---|
| χ2/dof | 54/35 | 37/47 | 49/41 | 113/83 |
| Γ |
 |
(1.9) | (1.9) | (1.9) |
| NPL [photons keV−1 cm−2] |
 |
 |
 |
 |
| log(NH/cm−2) |
 |
 |
 |
 |
| Covering Factor | (0.5) | (0.5) |
 |
(0.5) |
| fs [%] |
 |
 |
 |
 |
| Eline [keV] | − |
 |
− | 1.74 ± 0.03 |
| EWline [eV] | − |
 |
− |
 |
| kT1 [keV] |
 |
0.12 ± 0.01 |
 |
 |
| Nmekal1 [photons keV−1 cm−2] |
 |
4.4 ± 1.1 × 10−5 |
 |
1.6 ± 0.2 × 10−4 |
| kT2 [keV] |
 |
0.63 ± 0.03 |
 |
0.64 ± 0.02 |
| Nmekal2 [photons keV−1 cm−2] | 3.4 ± 0.9 × 10−6 | 7.0 ± 0.6 × 10−6 |
 |
2.20 ± 0.14 × 10−5 |
 [erg cm−2 s−1] |
6.1 × 10−14 | 3.1 × 10−14 | 2.1 × 10−14 | 1.6 × 10−13 |
 [erg cm−2 s−1] |
5.2 × 10−13 | 1.1 × 10−11 | 4.7 × 10−11 | 8.2 × 10−12 |
Notes. To fit the XMM-Newton spectrum of NGC 6323 we used the Cash statistic (Cash 1979), due to the low number of photons which were rebinned to be at least 3 counts per bin. All the other spectra were fitted with the χ2 statistic.
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