Table 1
Pulsars without confirmed TeV PWNe.
| PSR name | P | P | Ė | τc | PWN? | PWN/composite | Energy | Refs. |
|---|---|---|---|---|---|---|---|---|
| (10−2 s) | (10−14 s s−1) | (1036 erg s−1) | (kyr) | SNR name | band | (see also other refs. therein) | ||
| J0540-6919 | 5.06 | 47.9 | 146 | 1.67 | Y | G279.7-31.5 | R, X, O, G? | Manchester et al. (1993); Mignani et al. (2012); Bamba et al. (2022) |
| J0940-5428 | 8.75 | 3.29 | 1.93 | 42.2 | N | |||
| J1015-5719 | 14.0 | 5.74 | 0.828 | 38.6 | Y | G283.1-0.59 | R | Ng et al. (2017) |
| J1044-5737 | 13.9 | 5.46 | 0.803 | 40.3 | N | |||
| J1048-5832 | 12.4 | 9.61 | 2.00 | 20.4 | Y | X | Gonzalez et al. (2006) | |
| J1111-6039 | 10.7 | 19.5 | 6.35 | 8.66 | Y | G291.0-0.1 | R, X, G | Slane et al. (2012) |
| J1112-6103 | 6.50 | 3.15 | 4.53 | 32.7 | ? | X?, G? | Townsley et al. (2011); Ackermann et al. (2016) | |
| J1124-5916 | 13.5 | 75.3 | 11.9 | 2.85 | Y | G292.04+1.75 | R, X, G? | Ajello et al. (2017); Park et al. (2007); Gaensler & Wallace (2003) |
| J1135-6055 | 11.5 | 7.93 | 2.06 | 23.0 | Y | G293.8+0.6 | X, R? | Zhang & Bordas (2019); Bordas & Zhang (2020) |
| J1203-6242 | 10.1 | 4.41 | 1.71 | 36.1 | N | |||
| J1208-6238 | 44.1 | 327 | 1.51 | 2.14 | ? | X? | Bamba et al. (2020) | |
| J1341-6220 | 19.3 | 25.3 | 1.38 | 12.1 | ? | G308.8-0.1 | R?, G? | Acero et al. (2015); Green et al. (1997) |
| J1400-6325 | 3.12 | 3.89 | 50.7 | 12.7 | Y | X, R | Bamba et al. (2022); Renaud et al. (2010) | |
| J1410-6132 | 5.01 | 3.20 | 10.1 | 24.8 | ? | G312.4-0.4 | X? | Doherty et al. (2003) |
| J1524-5625 | 7.82 | 3.90 | 3.21 | 31.8 | N | |||
| J1637-4642 | 15.4 | 5.93 | 0.640 | 41.2 | ? | HESS J1640-465 | X?,G?, T? | Slane et al. (2010); Lemiere et al. (2009); Aharonian et al. (2006) |
| J1730-3350 | 14.0 | 8.48 | 1.24 | 26.1 | N | |||
| J1747-2958 | 9.88 | 6.13 | 2.51 | 25.5 | Y | Mouse | R,X | Klingler et al. (2018) |
| J1801-2451 | 12.5 | 12.8 | 2.59 | 15.5 | Y | Duck | R,X | Kaspi et al. (2001); Gaensler & Frail (2000) |
| J1813-1246 | 4.81 | 1.76 | 6.24 | 43.4 | ? | HESS J1813-126 | X?, T? | Marelli et al. (2014); Tibolla et al. (2022) |
| J1826-1256 | 11.0 | 12.1 | 3.58 | 14.4 | Y | Eel | X, G?, T? | Burgess et al. (2022); Roberts et al. (2007); Breuhaus et al. (2022) |
| J1837-0604 | 9.63 | 4.52 | 2.00 | 33.8 | ? | LHAASO J1839-0545 | T? | de Oña Wilhelmi et al. (2022); Cao et al. (2021) |
| J1838-0537 | 14.6 | 47.2 | 6.02 | 4.89 | ? | HESS J1841-055 | T? | MAGIC Collaboration (2020); Aharonian et al. (2008) |
| J1844-0346 | 11.3 | 15.5 | 4.25 | 11.6 | ? | HESS J1843-033 | T? | Sudoh et al. (2021); Devin et al. (2021); Amenomori et al. (2022) |
| J1932+2220 | 14.5 | 5.76 | 0.754 | 39.8 | N | |||
| J1934+2352 | 17.8 | 13.1 | 0.908 | 21.6 | N | |||
| J1935+2025 | 8.01 | 6.08 | 4.66 | 20.9 | ? | G054.1+00.3 | X?, T? | Temim et al. (2010); Xia et al. (2023) |
| J2021+3651 | 10.4 | 9.57 | 3.38 | 17.2 | Y | G75.2+0.1 | R, X, T? | Roberts et al. (2008); Woo et al. (2023); Abeysekara et al. (2020) |
| J2022+3842 | 4.86 | 8.61 | 29.6 | 8.94 | Y | G076.9+1.0 | R, X | Arzoumanian et al. (2011); Marthi et al. (2011) |
| J2111+4606 | 15.8 | 14.3 | 1.44 | 17.5 | N | |||
| J2229+6114 | 5.16 | 7.83 | 22.5 | 10.5 | Y | Boomerang | R, X, G, T? | MAGIC Collaboration (2023); Pope et al. (2024) |
| J2238+5903 | 16.3 | 9.70 | 0.889 | 26.6 | N |
Notes. The parameters in Cols. 2, 3, 4, and 5 are from the ATNF catalog2 (Manchester et al. 2005). The “Y” in column 6 indicates that its PWN has been confirmed in one or several bands; an “N” means that the PWN has not been observed yet to our knowledge; and a question mark means that there is a possible PWN counterpart in some band or bands but that it has not yet been confirmed. In the eighth column (PWN energy band), “R, O, X, G, T” stand for radio, X-rays, visible, GeV, and TeV energy ranges.
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