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Fig. 1


Rotation period versus its time derivative (“P- diagram”) for all known neutron stars. Lines of constant spin-down rate are shown and labeled. The small dark blue and medium light amber dots denote the known neutron stars not in our database, and the neutron stars in our database with no detected glitches, respectively. The large orange and turquoise dots represent those pulsars in our database with large glitches, and only small glitches detected, respectively. The turquoise triangles correspond to the magnetars in our database, which only have small glitches detected. P and for neutron stars not in our database were taken from the ATNF pulsar catalog 2 (Manchester et al. 2005).

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