Table 2
Pulsars for which one or more glitches occurred during the range of the ephemerides used in this paper (above the horizontal line) or near the range of validity of our ephemerides (below the horizontal line).
| PSR Name | Start | End | Glitch epoch |
| [MJD] | [MJD] | [MJD] | |
|
|
|||
| B0355+54 | 51 364.6 | 56 262.2 | 51 679(15)[1] |
| 51 969(1)[1] | |||
| 52 943(3)[1] | |||
| 53 209(2)[1] | |||
| B0525+21 | 52 274.9 | 56 641.1 | 52 296(1)[2,3] |
| 53 379[2] | |||
| 53 980(12)[3] | |||
|
|
|||
| B0919+06 | 55 555.2 | 56 557.5 | 55 152(6)[1] |
| B1530+27 | 51 607.0 | 56 535.6 | 49 732(3)[1] |
| B1822−09 | 54 876.5 | 56 571.8 | 54 114.96(3)[1] |
| B1907+00 | 54 984.1 | 56 556.9 | 53 546(2)[1] |
| B1907+10 | 54 924.5 | 56 535.1 | 54 050(350 [s])[3] |
| B2224+65 | 55 359.7 | 56 570.1 | 54 266(14)[2,3] |
| B2334+61 | 54 635.4 | 56 507.3 | 53 642(13)[1,3] |
Notes. The uncertainty of the glitch epoch is quoted in parentheses and it is expressed in days, except for the case of PSR B1907+10, where it is quoted in seconds. Sources: Jodrell Bank and ATNF glitch archives.
Reference. [1] Espinoza et al. (2011); [2] Janssen & Stappers (2006); [3] Yuan et al. (2010).
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