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Table 4

Results of spectral fits.

Model  (d.o.f.) Null Hyp. NH Parameter FX Comment
(%) (1021 cm-2) (erg s-1 cm-2)

[1] bbody 1.66(61) 0.091 k T 138(3) eV Wilms et al. abundances
[2] bbody 2.22(61) 1.3 × 10-5 2.76(23) k T 152(3) eV 5.9(4) × 10-13 Hamaguchi et al. abundances
[3] bbody 1.21(60) 13 k T 124(4) eV 1.20(22) × 10-12 ZO = 1.66(12) (solar)

[4] nsa B0 1.64(61) 0.114 T eff K M   = 1.4 M, R   = 10 km
[5] nsa B0 1.70(59) 0.067 4.25(18) T eff K M, R ~ 10 km a
[6] nsa B12 1.80(61) 0.013 T eff 7.1(3) × 105 K M   = 1.4 M, R   = 10 km
[7] nsa B12 1.43(59) 1.673 T eff K M ~ 2 M, R ~ 7 km b
[8] nsa B13 1.98(61) 7.6 × 10-4 T eff K M   = 1.4 M, R   = 10 km

[9] powerlaw 2.37(61) 9.1 × 10-7 9.9(4) Γ 8.58(26) 8(5) × 10-7 Wilms et al. abundances

[10] bbody-gauss 1.05(57) 38 2.7(3) k T eV ZO = 1.64(15) (solar)
ϵ keV σ = 0.14(1σ),EW = 91 eV
[11] bbody-2*gauss 1.01(58) 46 2.61   k T 134.9(2.4) eV 7.3(4) × 10-13 Wilms et al. abundances
ϵ 1 keV σ = 0.1  ,EW = 71 eV
ϵ 2 1.35(4) keV σ = 0.1  ,EW = 86 eV
[12] bbody-2*gauss 1.00(57) 48 2.2(3) k T 141(6) eV Wilms et al. abundances
ϵ 1 keV σ = 0.1  ,EW = 71 eV
ϵ 2 1.35(3) keV σ = 0.1  ,EW = 104 eV
[13] bbody+bbody 1.17(59) 17 5.2(6) 37(4) eV  kmc
119(4) eV  kmc
[14] bbody+pow 1.66(61) 0.091 2.61   k T eV 6.8(3) × 10-13 Wilms et al. abundances
Γ 1.7   − 2.1   d

Notes. Parameters marked with a star are held fixed during fitting.

(a)

Stellar radius unconstrained by the model.

(b)

Stellar mass and radius unconstrained by the model.

(c)

Computed for distance d = 2.3 kpc.

(d)

Upper limit to the unabsorbed flux of the power-law component, in units of erg s-1 cm-2 (0.1 − 12 keV).

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