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Table 3.

X-ray spectral fitting results for both candidates.

BB

Source NH kT Radius (a) log(Z) log(ZBB/Z) AIC Absorbed flux (b)
[1020 cm−2] [eV] [km] [10−13 erg s−1 cm−2]
J0657 −37.4 0 65.7
J1317 −71.2 0 128.5

apec(c)

Source NH kT z log(Z) log(ZBB/Z) AIC Absorbed flux (b)
[1020 cm−2] [eV] [10−13 erg s−1 cm−2]

J0657 0 −39.5 2.0 68.0
J1317 −72.1 0.9 118.9

PL

Source NH Γ log(Z) log(ZBB/Z) AIC Absorbed flux (b)
[1020 cm−2] [10−13 erg s−1 cm−2]

J0657 −40.3 2.9 68.9
J1317 −83.7 12.5 151.2

NSA(d)

Source NH kT Magn. field Dist. log(ZBB/Z) AIC Absorbed flux (b)
[1020 cm−2] [eV] [G] [pc] [10−13 erg s−1 cm−2]

J0657 0 1.4 67.1
J0657 1012 1.2 66.6
J0657 1013 1.5 66.4
J1317 0 4.1 135.1
J1317 1012 2.9 133.4
J1317 1013 3.1 133.3

Notes. We present the median value estimated from the sample parameter distribution and the errors give the 1σ confidence region. We adopted 400 live points to sample the parameter space.

(a)

We assumed a 1 kpc distance for the blackbody emission radius at infinity.

(b)

The absorbed model flux covers the 0.2–10 keV range.

(c)

The abundance is fixed to the solar value.

(d)

We assume a canonical neutron star with 1.4 M and 12 km radius.

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