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. Author manuscript; available in PMC: 2020 Nov 3.
Published in final edited form as: Mon Not R Astron Soc. 2020 Sep 1;498(4):4605–4614. doi: 10.1093/mnras/staa2640

Table 1.

PSR J0537–6910 timing model parameters for segments between glitch epochs. Number in parentheses is 1σ uncertainty in last digit.

Segment Epoch (MJD) Start (MJD) End (MJD) TOAs v (Hz) (10−10 Hz s−1) (10−20 Hz s−2) nig Residual RMS (μs) χ2/dof
0 58020 57984.5 58057.5 4 61.924374260(2) −1.99547(5) [1]a 66.14 3.1
1 58124 58108.1 58141.6 3 61.922597203(3) −1.9961(3) [1]a 1.158 b
2 58255 58163.0 58348.8 21 61.9203729962(9) −1.996977(2) 0.56(1) 8.7(2) 123.5 4.4
3 58399 58377.5 58422.2 11 61.917896251(3) −1.99689(2) 5.9(6) 90(10) 56.39 1.2
4 58493 58426.1 58560.6 13 61.916299559(4) −1.997261(8) 0.81(8) 13(1) 250.8 20
5 58600 58571.3 58629.3 7 61.914462421(2) −1.99740(3) [1]a 98.49 3.3
6 58723 58645.5 58804.5 16 61.912366620(2) −1.997289(4) 0.88(3) 13.7(4) 142.7 5.9
7 58836 58810.0 58862.9 6 61.910424210(6) −1.99742(4) 5.8(9) 90(10) 81.92 4.7
8 58918 58872.5 58964.4 14 61.909033102(3) −1.99765(1) 1.4(1) 22(2) 138.4 6.9
a

is fixed at 10−20 Hz s−2 (see text).

b

No fit performed (see text).