Extended Data Fig. 4: Results from the ground-based campaign to detect HD 110067 f.
From: A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067
a, ΔWAIC for each of the constrained period bins when compared with a transit-free model. b,c, Best-fit decorrelated photometry with (b) and without (c) a transit model. Each light curve from each telescope has been offset for clarity. Error bars represent 1σ uncertainties.
