Central eclipse time posteriors from a joint-fit of all three eclipses using a shared eclipse depth but separate eclipse times. These posteriors were approximated using the median and 1σ upper and lower uncertainties (highlighted in orange) and used to constrain the eclipse times when fitting individual eclipses. The predicted eclipse time was calculated using values in Table D.1 but assumes a circular orbit and has been adjusted for light delay. All observations favour the eclipse to occur slightly early.