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Table 3
Results for the pulsar parameters fW0 and γ for the best fits in the single pulsar approach.
Name | Age [kyr] | Distance [kpc] | fW0 [ 1054 GeV ] | γ | χ 2 |
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p |
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0 | (2.95 ± 0.07) × 10-3 | 1.45 ± 0.02 | 23.4 | 0.57 | 0.99 | ||
J1745−3040 | 546 | 0.20 | (3.03 ± 0.06) × 10-3 | 1.54 ± 0.02 | 33.6 | 0.82 | 0.79 |
1.3 | 1 | 2.54 | 9902 | 241 | 0 | ||
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0.17 | (1.48 ± 0.03) × 10-3 | 1.56 ± 0.02 | 26.8 | 0.65 | 0.96 | ||
J0633+1746 | 342 | 0.25 | (1.63 ± 0.02) × 10-3 | 1.68 ± 0.02 | 49.6 | 1.21 | 0.17 |
Geminga | 0.48 | (1.01 ± 0.06) × 10-2 | 2.29 ± 0.02 | 332 | 8.10 | 0 | |
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0.10 | (2.28 ± 0.05) × 10-3 | 1.48 ± 0.02 | 21.7 | 0.53 | 0.99 | ||
J0942−5552 | 461 | 0.30 | (2.61 ± 0.04) × 10-3 | 1.69 ± 0.02 | 61.0 | 1.49 | 0.02 |
1.1 | 1 | 2.65 | 7747 | 189 | 0 | ||
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0 | (2.13 ± 0.05) × 10-3 | 1.46 ± 0.02 | 19.8 | 0.48 | 0.99 | ||
J1001−5507 | 443 | 0.30 | (2.49 ± 0.03) × 10-3 | 1.70 ± 0.02 | 62.4 | 1.52 | 0.02 |
1.4 | 1 | 2.46 | 13 202 | 322 | 0 | ||
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0.1 | (0.80 ± 0.02) × 10-3 | 1.52 ± 0.02 | 21.0 | 0.51 | 0.99 | ||
J1825−0935 | 232 | 0.30 | (1.45 ± 0.03) × 10-3 | 1.94 ± 0.02 | 126 | 3.07 | 0 |
1.0 | 1 | 2.64 | 12 776 | 312 | 0 | ||
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0.25 | (1.06 ± 0.05) × 10-3 | 2.18 ± 0.02 | 216 | 5.27 | 0 | ||
J0659+1414 | 111 | 0.28 | (2.53 ± 0.16) × 10-3 | 2.37 ± 0.02 | 316 | 7.71 | 0 |
Monogem | 0.31 | (7.96 ± 0.61) × 10-3 | 2.58 ± 0.02 | 444 | 10.8 | 0 | |
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0.26 | (2.53 ± 0.08) × 10-1 | 3 | 14 316 | 349 | 0 | ||
J0835+4510 | 11.3 | 0.28 | (3.90 ± 0.14) × 10-1 | 3 | 14 982 | 365 | 0 |
Vela | 0.3 | (6.00 ± 0.26) × 10-1 | 3 | 15 446 | 377 | 0 |
Notes. Only pulsars with a p-value > 0.0455, taking their distance uncertainty into account, are listed, besides the well-known pulsars Monogem and Vela. The bold lines correspond to the nominal distance value.
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