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Table 3.
Continuum parameters of the spectrum during the persistent emission and the power-law parameters resulting from the eclipsed spectrum.
| Continuum | Parameter (Unit) | Value |
|---|---|---|
| component | ||
| powpersistent | norm 1044 (ph s−1 keV at 1 keV) | 1.6 ± 0.02 |
| Γ (photon index) | 1.4 ± 0.01 | |
| bbpersistent | norm (cm2) |  |
| Temperature (keV) |  |
|
| poweclipsed | norm 1044 (ph s−1 keV at 1 keV) | 0.032 ± 0.003 |
| Γ | 1.9 ± 0.2 | |
Notes. The symbol “pow” refers to the power-law parameters and “bb” to the black body.
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