Pulsar glitches

Example of a glitch
A glitch in the data of the Crab pulsar. It occurred in March 2003 and is the largest detected glitch on this pulsar. However, it is small compared to the glitches observed in Vela-like pulsar, which are about 1,000 times larger. Check the paper for more details.

Pulsars are famous for their very stable rotation, provided by their high density and rapid spin. Pulsar timing, the method by which the rotation of pulsars is measured and described, is a high precision discipline. This accuracy makes it possible to detect and measure very small perturbations affecting the normal rotation of the star.

Glitches are rare events of very short duration, seen in the data as sudden jumps in rotational frequency. Following a glitch, the pulsar sometimes enters a stage of recovery, in which the rotation frequency decays towards the pre-glitch value.

Glitch Catalogue

The catalogue contains basic glitch information on all published glitches plus regularly updated detections using the Lovell telescope at Jodrell Bank Observatory (view the table).

Should you have comments, questions or suggestions, please contact Cristóbal Espinoza
(cme -at- jb.man.ac.uk).

Please refer to Espinoza et al. (2011)
and the url http://www.jb.man.ac.uk/pulsar/glitches.html
when using this data for publications.