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Table B.1.
Results of the neutron star atmosphere model fitting.
| Detection | B = 2 × 1012 G | |||||
|---|---|---|---|---|---|---|
| ObsID | Exposure | Distance | LogTeff | Remission | FX | LX |
| (ks) | (kpc) | (10−2 K) | (10−2 km) | (10−14 erg cm−2 s−1) | (1032 erg s−1) | |
| 16723 | 26.9 | 12 | 711.2 |
2.72 |
1.63 |
2.81 |
| " | " | 22 | " | 5.0 |
" | 9.4 |
| 16725 | 28.6 | 12 | 712 |
1.5 |
0.54 |
0.94 |
| " | " | 22 | " | 2.7 |
" | 3.2 |
| 16726 | " | 12 | 712.5 |
1.94 |
1.06 |
1.83 |
| " | " | 22 | " | 3.6 |
" | 6.1 |
Notes. The value of the absorption column was fixed to 1.03 × 1022 cm−2 (Kalberla et al. 2005). The spectral parameters, fluxes and luminosities have been calculated in the 0.5–10 keV energy range. The errors are 1σ.
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