Table 1
Best-fitting X-ray spectral parameters of PID352 derived from XMM-Newton and Chandra (CDF-S and E-CDF-S).
| Data | Γsoft | Γhard | NH | z | E Wem.line | Eabs.line | E Wabs.line | F2−10 keV | L 2−10 keV | χ2(C)/d.o.f. | |
| (× 1023 cm-2) | (eV) | (keV) | (eV) | (erg cm-2 s-1) | (erg s-1) | ||||||
|
|
|||||||||||
| X | 1.73 ± 0.31 | 1.58 |
2.30 |
1.59 ± 0.03 | 76 ± 35 | 2.94 ± 0.04 | −82 |
2.6–3.1–2.8 | 3.5–4.2–3.8 | 275.3/268 | |
| C | ... | 1.03 |
1.01 |
1.62 ± 0.05 | 120 |
2.85 |
−65 |
2.4–3.6 | 1.9–2.8 | 350.0/480 | |
Notes. X: XMM-Newton (pn, MOS1, and MOS2); C: Chandra (CDF-S 4Ms+E-CDF-S data). Both line energies and equivalent widths are reported in the observed frame, while the column density is given at the reported best-fitting redshift solution. Fluxes are reported in the observed 2–10 keV band (units of 10-14), while luminosities are intrinsic (i.e., corrected for obscuration) and in the restframe 2–10 keV band (units of 1044). The three fluxes and luminosities reported for XMM-Newton refer to pn, MOS1, and MOS2 data, respectively, while for Chandra the two fluxes and luminosities refer to CDF-S and E-CDF-S data, respectively. Both emission and absorption lines were modeled using a Gaussian feature of width σ = 10 eV.
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