Table 1.
Best-fitting parameters for the June 9 XMM, June 16–21 Swift/XRT, and Nov. 30, 2016 XMM spectra.
| ID | TTH (eV) | KTH | Γ | FPL [0.3 − 1] | FTH [0.3 − 1] | FTH, bol | χ2/d.o.f. | C/d.o.f. |
|---|---|---|---|---|---|---|---|---|
| June 9 XMM-Newton spectrum | ||||||||
| BB |
 |
 |
... | ... |
 |
 |
7.35/7 | ... |
| DISKBB |
 |
 |
... | ... |
 |
 |
7.30/7 | ... |
| June 16–21 Swift/XRT spectrum | ||||||||
| BB | [52] |
 |
... | ... |
 |
 |
... | 10.90/25 |
| DISKBB | [64] |
 |
... | ... |
 |
 |
... | 10.45/25 |
| Nov. 30 XMM-Newton spectrum | ||||||||
| BB |
 |
 |
... | ... |
 |
 |
138.9/120 | ... |
| DISKBB |
 |
 |
... | ... |
 |
 |
120.3/120 | ... |
| BREMS |
 |
 |
... | ... |
 |
... | 114.5/119 | ... |
| DISKBB+PL |
 |
 |
[1.8] |
 |
 |
 |
109.3/119 | ... |
Notes. The Galactic absorption column NH was fixed to 1.9 × 1020 cm−2. The thermal models are denoted with temperatures TTH (in eV) and normalizations KTH that correspond to a black body (Tbb, Kbb), disk black body (Tdbb, Kdbb) and bremsstrahlung (Tbr, Kbr). The model normalizations are: Kbb = (Rbb[km]/d10)2, Kdbb = (Rdbb[km]/d10)2 cos i. The 0.3–1 keV band fluxes are not corrected for local or interstellar absorption and they are given in units of 10−13 erg cm−2 s−1.
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