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Fig. 1


Spin-down power Ė and γ-ray efficiency η as a function of the distance, for PSR J06102100. ĖShk denotes the Shklovskii correction to Ė, ĖGal is the contribution from the line of sight acceleration in the Galactic potential, and Ėint is the spin-down power obtained after correction for these effects. The blue curve represents the γ-ray efficiency, η (the y-axis scale is in percent), and the gray-shaded area shows the region excluded by the condition η> 0. Finally, the red dashed line shows the NE2001-predicted distance for PSR J06102100 of 3.54 kpc, and the green-shaded region represents the zone excluded by the 2σ lower limit on the distance from our timing analysis, of 0.77 kpc.

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