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Table 4

Best-fit spectral parameters of the orbital phase-resolved spectra from the standard sample.

Sample Cutoff PL + BB (Ecut = 20.1 keV fixed, kTBBb = 0.14 keV fixed)

Phase-bin φ1 φ2 φ3 φ4 φ5 φ6 φ7

NH/ 1022 cm-2
Γ
NormPL
χ2/d.o.f. 173/212 = 0.82 233/247 = 0.94 244/237 = 1.03 216/228 = 0.95 246/228 = 1.08 216/205 = 1.05 204/199 = 1.03

Model Partial covering

Phase-bin φ1 φ2 φ3 φ4 φ5 φ6 φ7

NH/ 1022 cm-2 0.+ 1.4
NHpc/ 1022cm-2
Cov. Fract.pc
Γ
NormPL
χ2/d.o.f. 192/211 = 0.91 250/247 = 1.01 248/236 = 1.05 212/227 = 0.94 251/227 = 1.11 237/204 = 1.16 219/198 = 1.11

Notes. The errors correspond to the 1σ-uncertainties.

(b)

Blackbody component.

(pc)

Partial Covering Model.

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