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Table 7.
Fluxes for the different emission components adopted to model the broadband emission of RBS 1332 assuming the two-coronae model.
| Diskbb | Warm corona | Hot corona | |
|---|---|---|---|
| (0.001–0.3 keV) | 0.3–2 keV | 2–10 keV | |
| Obs. 1 | −11.20 ± 0.02 | −11.20 |
−11.91 ± 0.09 |
| Obs. 2 | −11.19 ± 0.02 | −11.40 ± 0.05 | −11.87 ± 0.02 |
| Obs. 3 | −11.19 ± 0.02 | −11.10 ± 0.02 | −11.63 ± 0.01 |
| Obs. 4 | −11.19 ± 0.02 | −11.30 ± 0.05 | −11.75 ± 0.02 |
| Obs. 5 | −11.19 ± 0.02 | −11.67 ± 0.03 | −12.18 ± 0.03 |
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