X-ray and gamma-ray fluxes of high-confidence pulsar detections (filled circles), probable associations between pulsars and high-energy gamma-ray sources (open circles), and candidate radio-quiet pulsars (filled squares). All X-ray fluxes are given for the 0.1 to 2.4 keV energy band, in cases of different energy band quoted in the literature (Crab, B1509−58, B1951+32, B1046−58 from Becker & Trümper 1997, SAX J0635+0533 from Kaaret et al. 1999, AX J1420.1−6049 from Roberts et al. 2001, J0218+4332 from Kuiper et al. 1998), the flux is normalized into the chosen energy band. The gamma-ray fluxes are given above 100 MeV, in cases where different event selection criteria were used [B0656+14: >50 MeV (Ramanamurthy et al. 1996), B1046−58: >400 MeV (Kaspi et al. 2000), B1509−58: 30 to 100 MeV (Kuiper et al. 1999), J0218+4332: 100 to 300 MeV (Kuiper et al. 2000)] the appropriate gamma-ray flux above 100 MeV has been determined for the energy band desired here.