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This article has an erratum: [https://doi.org/10.1051/0004-6361/201731519e]


Table 1

Statistics of glitches for pulsars binned by their spin-down rate.

# Bin Ti N N t N pg N p
(Hzs-1) (yr)

1 −16.75 117 0 0 0 7
2 −16.25 430 0 0 0 25
3 −15.75 1233 0 0 0 70
4 −15.25 2478 0 3 3 139
5 −14.75 2675 0 11 8 142
6 −14.25 1973 0 25 16 105
7 −13.75 2083 0 35 20 113
8 −13.25 1706 1 29 18 105
9 −12.75 1312 3 26 14 81
10 −12.25 745 4 38 15 48
11 −11.75 493 8 74 15 33
12 −11.25 357 37 78 18 20
13 −10.75 66 13 19 5 5
14 −10.25 44 4 8 2 3
15 −9.75 16 0 2 1 1
16 −9.25 46 0 25 1 1

Notes. The first column is the bin number. The second and third columns correspond to for the group of pulsars in each bin (the central value of each logarithmic interval), and the sum of the observation time of all pulsars in that bin. The next two columns contain the number of large glitches and the total number of glitches, respectively. The last two columns correspond to the number of pulsars with glitches, and the total number of pulsars in each bin, respectively.

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