Table 2
Spectral parameters of the X-ray spectra of PBC J2333.9-2343 obtained by XMM-Newton using a power-law model and UV and optical photometry from the OM.
| Analysis | ObsID | Γ | Norm | Flux (2–10 keV) | L(2–10 keV) |
|
UVW1 | U | V |
| (×10-3) | (×10-11 erg s-1 cm-2) | (×1043 erg s-1) | (×10-16 erg s-1 cm-2) | ||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
|
|
|||||||||
| Individual | 0760990101 | 1.77 |
2.61 |
0.96 |
5.07 |
1.03 | 8.41 ± 0.13 | 7.01 ± 0.09 | 18.78 ± 0.19 |
| 0760990201 | 1.77 |
2.18 |
0.79 |
4.16 |
0.99 | 8.55 ± 0.12 | 6.70 ± 0.07 | 19.55 ± 0.14 | |
|
|
|||||||||
| Simultaneous | 0760990101 | 1.77 |
2.67 |
0.97 |
5.06 |
1.02 | |||
| 0760990201 | 2.23 |
0.78 |
4.23 |
||||||
Notes. Column 1: type of analysis, where individual means that each spectrum was analyzed, and simultaneous means that the two spectra are analyzed together (we note that the normalization of the power law is variable, therefore each of the lines correspond to the values of the spectral parameters of the observations in Col. 2), Col. 2: ObsID., Col. 3: spectral index, Col. 4: normalization of the power law, Cols. 5 and 6: X-ray intrinsic flux and luminosity in the 2–10 keV energy band, Col. 7: reduced χ2, and Cols. 8–10: fluxes from the OM in units of 10-16 erg cm-2 s-1. In all cases z = 0.0475 and NG = 1.63 × 1020 cm-2. The errors are indicated as interval limits and are estimated at the 90% confidence.
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