This article has an erratum: [https://doi.org/10.1051/0004-6361/201731519e]
A zoom-in to the zone plus the last three bins, with the highest values. The straight line shows the linear relation . The glitch activity of PSR J0537−6190 was plotted using a gray square to show that this young pulsar follows the general trend. The activity obtained when including this pulsar in the appropriate bin is represented by the gray dot.
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