Results of the Hare and Hound (injection and retrieval) exercise of an Earth-sized planet transiting a V = 10 Sun-like star. With an orbital period of 365.25 d the planet transits 4 times in the 3.3 yr simulated light curve. Top: Light curves observed with a single camera (coloured per quarter) and the corresponding Wōtan trend (white/black lines). Middle: detrended light of all 24 camera observations (black dots) with in-transit data highlighted (dots). Bottom: Phase folded light curve on the best fit period from TLS. For clarity a 1 h binned representation of the light curve is shown (pink circles), together with the injected variability (blue line), and a best fit transit model (orange line).