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Table 2.

X-ray spectral fitting results of Swift/XRT and XMM-Newton/pn spectra.

(1) (2) (3) (4) (5) (6) (7) (8) (9)
Model Γ Γ1 kT C-s/d.o.f. F0.3−2 keV F2−10 keV L0.3−2 keV L2−10 keV
10−14 10−14 1041 1041
[eV] [erg cm−2 s−1] [erg cm−2 s−1] [erg s−1] [erg s−1]
Swift/XRT (0.3–10 keV)

PL 3.9 3.81/8 5.23 0.14 1.74 0.05
PL+PL 4.8 0.9(fix) 1.17/6 5.65 3.01 1.92 0.90
PL+BB 0.9(fix) 78 0.75/6 5.11 3.71 1.67 1.11

XMM-Newton/pn (1–10 keV)

PL 0.9 2.12/7 3.32 0.94

XMM-Newton/pn (0.2–10 keV)

PL 2.4 19.54/25 1.65 0.67 0.52 0.22
PL+PL 3.7 0.9(fix) 8.57/22 1.64 2.84 0.52 0.85
PL+BB 0.9(fix) 90 9.13/22 1.59 3.35 0.50 1.00

Notes. Column (1), Fitting model, PL, PL+PL, and PL+BB are phabs*powerlaw, phabs*(powerlaw+powerlaw), and phabs*(power law+zbbody), respectively, in Xspec; the column density of phabs is fixed at the Galactic column density of NH = 1.82 × 1020 cm−2; Cols. (2)–(3), Photon index Γ of PL component; Col. (4), temperature kT of BB component; Col. (5), best fitting C-statistic/degree of freedom; Cols. (6)–(7), in 0.3–2 and 2–10 keV band after correcting the Galactic absorption; Cols. (8)–(9), luminosity in 0.3–2 and 2–10 keV band after correcting the Galactic absorption.

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