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Table 1.

Best-fit parameters of the spectral empirical models.

Model cPL cPL+dBB PC*cPL PC*(cPL+dBB) PC*(cPL+dBB)

Parameter Value Units
NH Gal (a) 4 (fixed) 4 (fixed) 4 (fixed) 4 (fixed) 4 (fixed) 1020 cm−2
NH SMC (a) →0 →0 →0 →0 < 3 1020 cm−2
TBpcf NH 1022 cm−2
cov. frac. 45 ± 3 45 ± 3 %
dBB (b) kTBB 0.07 (fix) keV
NormBB 6.3−0.6+5.3 sin θ (RBB/D10)2
cPL (c) Γ 0.85 ± 0.02 1.05 ± 0.03
Ec 20.6 ± 0.9 keV
Norm (c) 101 ± 2 10−12 erg cm−2 s−1
Other information
Total fit stat./d.o.f. 1399.56/1035 954.11/1033 940.51/1033 923.36/1031 940.47/1032
Goodness (d) 100% 4% 1% 0% 4%

LX(e) 4.67 ± 0.08 4.13 ± 0.08 5.03 ± 0.08 4.6 ± 0.2 5.03 ± 0.10 1037 erg s−1
(e) 2.60 ± 0.03 2.30 ± 0.04 2.80 ± 0.04 2.55 ± 0.13 2.8 ± 0.05 1017 g s−1

Notes.

(a)

Galactic absorption was fixed to this value (see text for details).

(b)

The disk blackbody (diskbb in xspec) radius may be estimated from the normalisation of the model and a distance of 62 kpc (i.e., D10 = 6.2) assuming a disk inclination angle θ.

(c)

Cut-off power law (cut-offpl in xspec), where the normalisation is the unabsorbed X-ray flux in the 0.3–80 keV band.

(d)

Based on XSPEC simulations, denotes the percentage of simulated spectra that when fitted with the same model yield lower test statistics than the data.

(e)

Unabsorbed X-ray luminosity (0.3–80 keV) for a distance of 62 kpc for the cut-off power-law component. Mass-accretion rate onto the NS, assuming LX = 0.2 Ṁc2.

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