Table 1.
Number of known canonical pulsars, with spin-down luminosity, Ė, above and below 1028 W, and above 1031 W.
| log(Ė) (W) | Ntot | Nr | Ng | Nrg |
|---|---|---|---|---|
| > 31 | 4 | 0 | 2 | 2 |
| > 28 | 150 | 40 | 44 | 66 |
| Total | 2193 | 2020 | 80 | 93 |
Notes. The quantities Nr, Ng, and Nrg are the number of radio-only, gamma only, and radio-loud γ-ray pulsars, respectively. It should be noted that we excluded the binary pulsars, the pulsars in the Magellanic clouds and in globular clusters, then we selected the pulsars with a magnetic field between 6 × 106 T and 4.4 × 109 T. The data have been taken from the ATNF catalogue from https://www.atnf.csiro.au/research/pulsar/psrcat/
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