All Tables

Table 1: Pulsed X-ray properties of rotation-powered pulsars. Comparison of model X-ray luminosity ( $L^{\rm th}_{\rm X}$ ) (assuming $\alpha =55^{\circ }$ ) with observed pulsed X-ray luminosity ( $L^{\rm ob}_{\rm X}$ ) for each X-ray pulsars.
Table 2: Comparison of observed and theoretical $\gamma$ -ray luminosity for confirmed high-energy $\gamma$ -ray pulsars.