Table 1
Best-fit parameters of IGR J18410-0535 during different time intervals of the XMM-Newton observation (see Fig. 1 and the note below the table).
| Interval | Tstart | Tstop | Exp. | N H | Γ | Eline | EWline | Fobs | Funabs |  /d.o.f. |
| (s) | (s) | (ks) | (1022 cm-2) | (keV) | (keV) | (erg cm-2 s-1) | (erg cm-2 s-1) | (C-statistics/d.o.f.) | ||
|
|
||||||||||
| A | 0 | 3200 | 2.7 | 2.6 |
1.3 |
– | – | 3.2 × 10-13 | 4 × 10-13 | (12.4/11) |
| B | 3200 | 4670 | 1.2 | 8.0 |
1.1 ± 0.9 | – | – | 1.7 × 10-12 | 2.8 × 10-12 | (14.4/18) |
| C | 4670 | 5020 | 0.35 | 19.3 |
2.2 ± 0.7 | – | – | 1.0 × 10-11 | 5.0 × 10-11 | (51.0/47) |
| D | 5020 | 5220 | 0.17 | 19.8 |
1.9 ± 0.7 | – | – | 6.0 × 10-11 | 2.4 × 10-10 | 0.8/12 |
| E | 5220 | 6320 | 0.96 | 10.8 |
1.1 ± 0.1 | 6.56 ± 0.05 | 0.06 | 3.2 × 10-10 | 6.0 × 10-10 | 1.0/149 |
| F | 6320 | 6820 | 0.44 | 10.9 |
1.1 ± 0.1 | – | – | 2.9 × 10-10 | 5.3 × 10-10 | 0.9/109 |
| G | 6820 | 7620 | 0.7 | 12.4 |
1.4 ± 0.2 | – | – | 2.2 × 10-10 | 4.4 × 10-10 | 1.1/108 |
| H | 7620 | 8520 | 0.8 | 11.8 |
1.5 ± 0.2 | – | – | 1.3 × 10-10 | 2.9 × 10-10 | 1.1/73 |
| I | 8520 | 9520 | 0.9 | 15.5 |
1.6 ± 0.2 | 6.32 ± 0.05 | 0.10 | 6.2 × 10-11 | 1.8 × 10-10 | 0.8/107 |
| J | 9520 | 10420 | 0.8 | 14.3 |
1.2 ± 0.2 | – | – | 8.4 × 10-11 | 1.9 × 10-10 | 0.8/110 |
| K | 10420 | 11520 | 1.0 | 17.0 ± 1.5 | 1.3 ± 0.2 | – | – | 6.5 × 10-11 | 1.6 × 10-10 | 1.1/114 |
| L | 11520 | 14520 | 2.6 | 23.3 ± 2.0 | 1.6 ± 0.2 | – | – | 2.3 × 10-11 | 8.5 × 10-11 | 1.0/102 |
| M | 14520 | 16620 | 1.8 | 28.0 |
1.7 ± 0.4 | – | – | 8.2 × 10-12 | 3.3 × 10-11 | 1.2/58 |
| N | 16620 | 18870 | 1.8 | 43.4 |
2.0 ± 0.6 | – | – | 5.1 × 10-12 | 5.3 × 10-11 | 1.4/36 |
| O | 18870 | 42840 | 20.8 | < 0.5 | -0.9 ± 0.3 | 6.36 ± 0.06 | 1.1 | 2.2 × 10-13 | 2.2 × 10-13 | 1.0/13 |
| O1 | 18870 | 22820 | 3.4 | < 8.0 | -1.8 |
6.33 ± 0.06 | 1.2 | 9.7 × 10-13 | 9.8 × 10-13 | 0.8/5 |
| O2 | 22820 | 42840 | 17.4 | < 1.4 | 0.3 |
– | – | 8.8 × 10-14 | 9.1 × 10-14 | (12.5/10) |
Notes. The continuum spectral model is an absorbed power law. Here, NH is the absorption column density, Γ is the power-law photon index, Eline is the energy of the centroid of the iron line, and EWline the corresponding equivalent width. Fobs (Funabs) is the absorbed (unabsorbed) flux in the 1–10 keV band. In the last column we report the value of the /d.o.f. or the corresponding value of the C-statistics/d.o.f, for each spectrum.
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