Table 4
Results of the black body and power-law model for XMM-Newton spectra.
| Inst-Obsdate | Γ2−10 keV | kT | F BB | F PL | χ2/d.o.f. | ||
| (1) | (2) | (3) | (4) | (5) | (6) | ||
|
|
|||||||
| X-2012-10-18 | 1.57 ± 0.10 |
|
0.012 ± 0.005 | 0.216 ± 0.005 | 291.9/258 | ||
| X-2012-05-01 | 1.43 ± 0.19 |
|
0.023 ± 0.005 | 0.128 ± 0.004 | 134.3/131 | ||
| X-2004-04-11 | 1.39 ± 0.08 |
|
0.059 ± 0.009 | 0.383 ± 0.006 | 396.4/398 | ||
Notes. Best-fit parameters for the absorbed simple power law and black body. The absorption is fixed to its Galactic value, 3.17 × 1020 cm-2 (Kalberla et al. 2005). (1) Instrument and observation date. (2) Photon index, fitted in the (2−10) keV band and fixed for broad band analysis. (3) Black body temperature in keV. (4, 5) Absorption-corrected (0.5−2) keV flux in units of 10-12 erg cm-2 s-1 of the black body and the power law, respectively. (6) Fit statistics χ2 per degrees of freedom.
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