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Table 4
Best fit non-solar abundance models for the XRT spectra.
| Day | kT (BB) | kT (mekal) | N H | |
| after T0 | keV | keV | 1022 cm-2 | |
|
|
||||
| < 30 | 0.042 ± 0.003 | 4.10 |
1.55 |
|
| 30–60 | 0.064 |
1.99 |
0.62 ± 0.09 | |
| > 60 | ... | 0.80 |
0.69 |
|
|
|
||||
| Day | Obs flux | Unabs flux | Obs flux | Unabs |
| after T0 | total | total | hotter | hotter |
|
|
||||
| < 30 | 6.17E-12 | 2.44E-8 | 5.81E-12 | 1.09E-11 |
| 30–60 | 6.10E-12 | 6.99e-11 | 5.59E-12 | 1.17E-11 |
| > 60 | 1.34E-12 | 6.14E-12 | 1.34E-12 | 6.14E-12 |
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