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Table 1

Input parameters to our modelling and the corresponding spectral model used.

ATNF name RS NR RPWN Pt t Model E0 E1 Ecut E2 Γ Γ2 Refs.
(pc) (pc) (ms) (×10−13 s/s) (TeV) (TeV) (TeV) (TeV)
J1833–1034 2.98 0.8 61.8 2.02 BPL1 0.1 0.39 10 2.2 1,2
J1513–5908 38.4 19.2 151.6 15.3 BPL1 0.1 0.61 10 2.2 1,2
J1930+1852 10.8 2.7 136.9 7.50 BPL1 0.1 0.89 10 2.2 1,2
J1846–0258 2.6 0.58 326.6 71.1 BPL1 0.1 0.40 10 2.2 1,2
J0835–4510 19.5 12.2 89.3 1.25 BPL1 0.1 0.61 10 2.2 1,2
J1747–2809 19.8 2.5 52.2 1.56 BPL1 0.1 0.17 10 2.2 1,3
J2021+3651 103.7 0.957 PLEC 1 25 900 1400 1.4 4
J1841–0345 112.9 1.55 PLEC 1 × 10−5 7.0 72 740 2.2 5
J1849–0001 38.5 0.142 PL 0.5 10 100 2.5 6
J1826–1334 101.5 0.753 BPL2 0.7 0.9 42 1.4 3.25 7

Notes. RSNR and RPWN values are taken from Giacinti et al. (2020) and references therein. Pt and t values are taken from the ATNF catalogue (Manchester et al. 2005). The possible spectral models are described in Sect. 2, note that these models assume different radiation fields and should not be considered equivalent for all sources. References: (1) Giacinti et al. (2020), (2) H.E.S.S. Collaboration (2018a), (3) Aharonian et al. (2005), (4) Woo et al. (2023), (5) Albert et al. (2023), (6) Amenomori et al. (2023), (7) H.E.S.S. Collaboration (2019).

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