Table 1
Spectral models.
| # | NH | Γ | EFeKα | EWFeKα | Eabs | EWabs | F0.5–8 keV | F2–10 keV | χ2/d.o.f. |
|---|---|---|---|---|---|---|---|---|---|
| 1022 cm−2 | keV | eV | keV | eV | 10−13 erg s−1 cm−2 | 10−13 erg s−1 cm−2 | |||
| 1 | 3.86 |
1.75 |
6.37 |
105 |
3.82 | 3.29 | 333.5/349 | ||
| 2 | 3.71 |
1.73 |
6.37 |
94 |
9.22 |
235 |
306.4/347 | ||
| NH | Γ | EFeKα | EWFeKα | NH,ion | Log(ξ) | z | χ2/d.o.f. | ||
| 1021 cm−2 | keV | eV | 1021 cm−2 | ||||||
| 3 | 3.67 |
1.69 |
6.37 |
79 |
83 |
3. |
1.72 |
297.9/344 |
Notes. Upper table: Col. 1: model number; Col. 2: absorbing column in excess to the Galactic value; Col. 3: photon index; Col. 4: energy of the emission line; Col. 5:emission line rest frame EW; Col. 6: energy of the absorption line; Col. 7: absorption line EW; Col. 8: 0.5–8 keV flux; Col. 9: 2–10 keV flux; Col. 10: χ2/d.o.f. Lower table: Cols. 1–5 as in upper table. Col. 6: column density of the ionized absorber; Col. 7: log of the ionization parameter expressed in erg s−1 cm; Col. 8: observed redshift of the ionized absorber; Col. 10: χ2 /d.o.f. Line widths are fixed to 0 eV.
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