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Table 5

Best fits for the five pulsars selected in Sect. 4.1 as well as Monogem and Vela in the single pulsar approach, assuming the best propagation parameter set.

Name Age Distance fW0 γ K 0 L δ χ 2 p
[kyr] [kpc] [ 1054 GeV ] [ kpc2 Myr-1 ] [ kpc ]

J17453040 546 0.20 (3.02 ± 0.08) × 10-3 1.33 ± 0.01 0.00647 3.5 0.80 21.6 0.53 0.99

J0633+1746 342 0.25 (6.29 ± 0.08) × 10-4 1.74 ± 0.02 0.00850 2.0 0.60 18.0 0.44 0.99
Geminga

J09425552 461 0.30 (3.02 ± 0.08) × 10-3 1.34 ± 0.01 0.00647 3.5 0.80 21.6 0.53 0.99

J10015507 443 0.30 (3.02 ± 0.08) × 10-3 1.34 ± 0.01 0.00647 3.5 0.80 21.6 0.53 0.99

J18250935 232 0.30 (1.08 ± 0.07) × 10-3 2.18 ± 0.02 0.00802 1.5 0.55 23.0 0.56 0.99

J0659+1414 111 0.28 (6.20 ± 0.01) × 10-2 3.00 0.00590 1.0 0.55 63.7 1.6 0.01
Monogem

J0835+4510 11.3 0.28 1.00 2.49 ± 0.04 0.00335 1.0 0.65 3453 84 0
Vela

Notes. The pulsar ages and distances are the nominal values taken from the ATNF catalogue. The recently published positron fraction (Accardo et al. 2014) and the AMS-02 lepton spectrum (Weng et al. 2014) are used to derive the χ2, as in formula (20). The p-value, indicated in the last column, is defined in formula (22).

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