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Table 1
Hot structure parameters and the results from the fit.
| γ | δ |
|
|
|
|
|||
| 0 | 0.05 | 0.71 | 41.4 |
| 0.1 | 0.05 | 0.73 | 40.1 |
| 0.1 | 0.1 | 0.69 | 48.2 |
| 0.2 | 0.1 | 0.70 | 44.2 |
| 0.3 | 0.1 | 0.74 | 40.9 |
| 0.4 | 0.1 | 0.79 | 36.8 |
| 0.4 | 0.15 | 0.80 | 37.9 |
| 0.45 | 0.1 | 0.81 | 35.5 |
| 0.45 | 0.15 | 0.82 | 36.1 |
| 0.45 | 0.18 | 0.86 | 34.1 |
| 0.5 | 0.15 | 0.84 | 35.4 |
| 0.5 | 0.18 | 0.87 | 33.9 |
| 0.5 | 0.2 | 0.89 | 33.8 |
| 0.7 | 0.1 | 0.92 | 28.6 |
| 0.7 | 0.15 | 0.98 | 27.9 |
| 0.7 | 0.18 | 0.99 | 28.6 |
| 0.7 | 0.2 | 1.02 | 27.5 |
| 0.9 | 0.18 | 1.14 | 24.0 |
| 0.9 | 0.2 | 1.16 | 24.8 |
| 1 | 0.18 | 1.22 | 22.8 |
Notes. Thereal inner edge of the disk is at 45 km and the temperature is 0.7 keV. All of these models have an amplitude of modulations between zero and 20%; see Varniere & Vincent (2015a) for details on the calculation of the amplitudes.
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