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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

Figure 5.

Figure 5.

Timing residual for each merged observation after accounting for the best-fit timing model, with left axis in μs and right axis in fraction of rotation cycle. Errors are 1σ uncertainty. Segments are labeled by numbers and separated by the occurrence of a glitch, each of which is denoted by a vertical dashed line.