Table 3
Simple models fitted to the X-ray spectra of the two pulsars.
| Pulsar | Model | nH | kT | BB radius | Photon |
|
d.o.f. | F1/F2 | Flux |
| ( × 1022 cm-2) | (keV) | (km) | Index | ( × 10-14 erg cm-2 s-1) | |||||
|
|
|||||||||
| J1459−6053 | PL | 0.64 |
− | − | 2.10 |
1.16 | 12 | − |
|
| BB | 0.00 |
0.71 |
∗0.01 |
− | 1.48 | 12 | − |
|
|
|
|
|||||||||
| J1614−2230 | PL | 0.37 |
− | − | 4.64 |
0.94 | 77 | − | 2.68 |
| BB | 0.07 |
0.20 |
0.20 |
− | 1.04 | 77 | − |
|
|
| BB+PL | 0.24 |
0.13 |
0.74 |
1.25 |
0.83 | 75 | 0.41 |
|
|
| BB+BB | 0.20 |
0.15 and 0.88 |
0.53 and 0.01 |
− | 0.82 | 75 | 1.59 |
|
|
Notes. The errors quoted are at the 90% level. The quality of the fit (), the number of degrees of freedom (d.o.f.), the flux (F) ratio of the two components (1 and 2, when used) and the unabsorbed 0.2−10 keV flux are also shown. PL = power law, BB = blackbody, ∗ radius calculated for a reasonable distance estimate of 1 kpc.
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