Table 3
Pulsar wind nebulae outside the HGPS catalogue.
| Canonical name | ATNF name | lg Ė | τc | d | PSR offset | Γ | RPWN | L1-10 TeV |
|---|---|---|---|---|---|---|---|---|
| (kyr) | (kpc) | (pc) | (pc) | (1033 erg s-1) | ||||
| N157B1 | J0537−6910 | 38.69 | 4.93 | 53.7 | <22 | 2.80 ± 0.10 | <94 | 760 ± 80 |
| Crab Nebula2 | B0531+21 | 38.65 | 1.26 | 2.00 | <0.8 | 2.63 ± 0.02 | <3 | 32.1 ± 0.7 |
| G0.9+0.13 | J1747−2809 | 37.63 | 5.31 | 13.3 | <3 | 2.40 ± 0.11 | <7 | 46 ± 7 |
| 3C 584 | J0205+6449 | 37.43 | 5.37 | 2.00 | <2 | 2.4 ± 0.2 | <5 | 0.23 ± 0.06 |
| CTA 15 | J0007+7303 | 35.65 | 13.9 | 1.40 | <4 | 2.2 ± 0.2 | 6.6 ± 0.5 | 0.71 ± 0.10 |
Notes. See Table 1 for the explanation of the columns. G0.9+0.1 is listed in the catalogue, but not treated in the HGPS analysis pipeline, so we treat it as an HGPS-external result. Offset limits were calculated as for the HGPS (see Sect. 2.3). In the case of N157B and 3C 58, 2σPSF was used as conservativeextension limit since no value is given in the respective papers.
References. (1) H.E.S.S. Collaboration (2012c); Abramowski et al. (2015); (2) extension limit: Aharonian et al. (2004), flux: Aharonian et al. (2006b); (3) Aharonian et al. (2005a); (4) Aleksić et al. (2014); (5) Aliu et al. (2013).
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