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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 0.02 + 0.12 $ ^{+0.12}_{-0.02} $ −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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