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Table 3.

Best-fit parameters obtained from the fits of each set of data.

Data NH p Γ Nnorm1 Nnorm2 F(0.5−10) keV L(0.5−10) keV
tbabs*Model 1021 [cm−2] [keV] [keV] [erg s−1 cm−2] [erg s−1]
XMM-01

diskbb+pl 2.11 × 10−12 4.45 × 1039 748/703(1.06)
diskpbb 2.16 × 10−12 4.56 × 1039 752/704(1.07)
diskbb+nthcomp 1.80 × 10−12 3.80 × 1039 743/702(1.06)
diskbb+diskpbb 1.86 × 10−12 3.92 × 1039 744/702(1.06)

Suz-H-06

diskbb+pl 5.35 × 10−12 1.13 × 1040 599/553(1.08)
diskpbb 5.62 × 10−12 1.19 × 1040 607/554(1.10)
diskbb+nthcomp 4.97 × 10−12 1.05 × 1040 594/552(1.08)
diskbb+diskpbb 6.52 × 10−12 1.38 × 1040 602/552(1.09)

Suz-L-06

diskbb+pl 3.79 × 10−12 7.99 × 1039 458/461(0.99)
diskpbb 3.66 × 10−12 7.72 × 1039 459/462(0.99)
diskbb+nthcomp 3.21 × 10−12 6.77 × 1039 454/460(0.98)
diskbb+diskpbb 4.56 × 10−12 9.62 × 1039 453/460(0.98)

XMM-13+NuSTAR-13

diskbb+pl 8.52 × 10−12 1.80 × 1040 2009/1859(1.08)
diskpbb 8.44 × 10−12 1.78 × 1040 2069/1860(1.11)
diskbb+nthcomp ∼1.00 7.88 × 10−12 1.66 × 1040 2018/1858(1.08)
diskbb+diskpbb 9.08 × 10−12 1.92 × 1040 2045/1858(1.10)

XMM-14

diskbb+pl 3.46 × 10−12 7.30 × 1039 477/467(1.02)
diskpbb 2.36 × 10−12 4.98 × 1039 498/468(1.06)
diskbb+nthcomp 3.15 × 10−12 6.65 × 1039 477/466(1.02)
diskbb+diskpbb 3.16 × 10−12 6.67 × 1039 478/466(1.03)

XMM-16+NuSTAR-16

diskbb+pl 3.65 × 10−12 7.70 × 1039 591/561(1.05)
diskpbb 3.41 × 10−12 7.20 × 1039 601/562(1.07)
diskbb+nthcomp ∼363 2.86 × 10−12 6.03 × 1039 603/560(1.08)

XMM-18F

diskbb+pl 2.81 × 10−12 5.93 × 1039 174/174(1.00)
diskpbb 1.54 × 10−12 3.25 × 1039 186/175(1.06)
diskbb+nthcomp ∼994 2.62 × 10−12 5.53 × 1039 174/173(1.01)
diskbb+diskpbb 2.10 × 10−12 4.43 × 1039 174/173(1.01)

XMM-18S

diskbb+pl 7.60 × 10−12 1.60 × 1040 2324/2146(1.08)
diskpbb 7.43 × 10−12 1.57 × 1040 2330/2147(1.09)
diskbb+nthcomp ∼1.10 7.28 × 10−12 1.54 × 1040 2331/2145(1.09)
diskbb+diskpbb 8.95 × 10−12 1.89 × 1040 2320/2145(1.08)

Notes. The Galactic absorption hydrogen column density is given in the second column. The parameter p is the index of the disk temperature radius relation, T(r) ∝ rp. Γ is the power-law photon index. For the nthcomp model, we tie the disk inner radius temperature to the temperature of the soft seed photons which are scattered in the thermal Compton process. kTe is electron temperature of the Compton-heated region. In the case of diskbb and diskpbb, the normalization is unitless: (rin/D10)2cos(θ). The normalization of the pl is ph keV−1 cm−2 s−1 at 1 keV. The flux given in ninth column is unabsorbed.

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