Fig. 6.
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One- and two-dimensional posterior distributions of the eclipse light-curve parameters from iteratively fitting the FULLBAND data with the ±0.72° cuts where the precession rate was either fixed to the GR predicted value (green) or allowed to be fit as a free parameter (orange). Contours indicate the 68, 95 and 99.7% confidence intervals. Dashed black line is the predicted value of 
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