Notes. ^(a) The pulsar characteristic age is used for the age of the system, except where historical values are known. ^(b) Associated pulsar (PSR). Pulsar properties are taken from Manchester et al. (2005). ^(c) Putative pulsar candidate identified without pulsed emission detected by Temim et al. (2009). ^(d) Unknown quantities are marked by “?”. ^(e) R_PWN is the size of the PWN in radio (as opposed to the radio SNR shell). ^(f) v × t is the pulsar kick velocity multiplied by the age of the system, where a value of 300 km s⁻¹ is adopted for the velocity, corresponding to the average of known values (Hansen & Phinney 1997). ^(g) R_TeV is the one sigma radius taken from Abdalla et al. (2018b) for sources within the H.E.S.S. Galactic Plane Survey (HGPS), unless a reference is provided. ^(h)Stage of system evolution is assigned loosely based on age, which corresponds to Fig. 1. References. I: Frail et al. (1995), Kargaltsev et al. (2015), II: Caswell et al. (1981), Du Plessis et al. (1995), Trussoni et al. (1996), Mineo et al. (2001); III: Matheson & Safi-Harb (2010), Safi-Harb et al. (2001); IV: Green (2014), Green (2017), Dubner et al. (2008), Porquet et al. (2003); V: Duncan et al. (1996), Dwarakanath (1991), Tibaldo et al. (2018); VI: Ma et al. (2016), Temim et al. (2015); VII: Stupar et al. (2008), Duvidovich et al. (2019), Pavlov et al. (2008), Uchiyama et al. (2009); VIII: Pellizzoni et al. (2011), Abeysekara et al. (2017a), Posselt et al. (2017), Caraveo et al. (2003).