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Fig. 16.

image

Correlation between the GRAVITY fringe tracker residuals and the P5%/P95% injection stability metric, comparing STRAP and NAOMI. With NAOMI, the fringe tracking residuals tend to stay in the 80 nm–150 nm range because the P5%/P95% >  0.5 injection stability is high. This figure does not include 20% of the open-dome nights with wind speeds higher than 9 m s−1, where telescope vibrations affect fringe tracking residuals (Woillez et al. 2016).

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