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Table 2.

Updated parameters for all glitches detected by PuMA collaboration between MJD 58832 and MJD 60411.

PSR Age Glitch epoch Δνg/ν Δ ν ˙ g / ν ˙ $ \Delta \dot{\nu}_g / \dot{\nu} $ Δ ν ¨ / ν ¨ $ \Delta \ddot{\nu} / \ddot{\nu} $ Q τd References
(kyr) (MJD) (10−9) (10−3) (10−3) (d)
J0742–2822 157 59839.4(5) 4295(1) 72(1) 0.446(1)% 33.4(5) Zubieta et al. (2023)

J0835–4510 11 59417.6194(2) 1248(1) 83(4) –778.5(5) 0.7(1)% 0.994(8) Zubieta et al. (2023)
0.2(1)% 6.400(2)
41(1)% 535(8)
59479.0(2.5) 0.20(2) 0.13(1) This work

J1048–5832 20 59203.9(5) (#9) 8.90(9) 0.62(1) Zubieta et al. (2023)
59540(2) (#10) 9.9(3) Zubieta et al. (2023)
59732.9(1) (#11) 0.91(4) 0.009(8) This work
60090(10) (#12) 4.5(1) 1.01(4) This work
60406.6(5) (#13) ( † ) 4078(10) 11.0(5) Zubieta et al. (2024a)

J1740–3015 21 59935.1(4) 329.4(2) 2.32(1) 4.43(1)% 124(2) Zubieta et al. (2023)

Notes. Numeration with (#) in PSR J1048–5832 glitches follows Liu et al. (2023). ( † )Very recent glitch.

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