|[kpc]||[ms]||[ky]||[erg/s]||[erg/cm2 s]||[erg/cm2 s]||[erg/s]||[erg/s]|
Notes. The luminosities of the pulsed emission L are calculated as with values for the distance d taken from the table, and the beaming fraction set to 1. F represent the pulsed flux. (a) Luminosities, fluxes, and efficiencies labeled with x are evaluated for the 2-100 keV band. (b) Luminosities, fluxes, and efficiencies labeled with are evaluated for the 0.1-10 GeV band. (c) The -ray energy flux of PSR B1509-58 in the 0.1-10 GeV band has been derived from the (total) photon flux values for the 100-300 and 300-1000 MeV bands as given in Kuiper et al. (1999) assuming a power-law shape with photon index of 2.5, and should be considered as an upper-limit to the pulsed flux of PSR B1509-58 in the 0.1-10 GeV band.
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