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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 9.

Figure 9.

Time to next glitch as a function of glitch size Δv. Circles with errors are NICER values, and points with errors are RXTE values, which are from Table 2 of Antonopoulou et al. (2018). Vertical dotted line indicates the size of glitch 8, which is the most recent NICER-detected glitch and for which the time to next glitch is not known yet. Errors in Δv are 1σ uncertainty. Solid and dashed lines show a linear fit of NICER and RXTE data with time to next glitch = 6.4 d (Δv/μHz) and time to next glitch = 23 d + 5.08 d (Δv/μHz), respectively, while shading shows correlation regions which fit 68 percent of glitches (see Section 4.2).