Table 9
Spectral parameters of a fit to the five Swift-XRT,
Swift-BAT, and Suzaku-XIS spectra of the giant
2012 November outburst (
, 2582 d.o.f.).
| TBnew | N H | 
× 1022 cm-2 |
| PL a | F PL,1 | 
× 10-9 erg s-1 cm-2 |
| F PL,2 | 
× 10-9 erg s-1 cm-2 |
|
| F PL,3 | 
× 10-9 erg s-1 cm-2 |
|
| F PL,4 | 
× 10-9 erg s-1 cm-2 |
|
| F PL,5 | 
× 10-9 erg s-1 cm-2 |
|
| F PL,Suz. | 
× 10-9 erg s-1 cm-2 |
|
| BBODY a | kT |  keV |
| F BB,1 | 
× 10-9 erg s-1 cm-2 |
|
| F BB,2 | 
× 10-9 erg s-1 cm-2 |
|
| F BB,3 | 
× 10-9 erg s-1 cm-2 |
|
| F BB,4 | 
× 10-9 erg s-1 cm-2 |
|
| F BB,5 | 
× 10-9 erg s-1 cm-2 |
|
| F BB,Suz. | 
× 10-9 erg s-1 cm-2 |
|
| Iron line | W neutral |  eV |
| W He - like |  eV |
|
| W H - like |  eV |
|
| Constants | c XIS0 |
|
Notes.
FPL,i is the 15–50 keV flux and FBB,i is the bolometric flux of the secondary black body of the ith Swift observation of 2012 November as listed in Table 1, scaled to the PCA via the detector calibration constant cXRT and cXIS3 (Table 3). The calibration constant cXIS0 had to be refitted. FPL,Suz. and FBB,Suz. are the corresponding fluxes obtained by the Suzaku observation.
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