Notes. We injected eclipses of f_{in j} = 150 ppm (expected signal based on the first observation), f_{in j} = 200 ppm, and f_{in j} = 300 ppm (expected bare rock signal). The second column indicates whether the injection was done at the expected secondary eclipse time (exp.) or in a more well-behaved part of the light curve (beh.). The third column shows whether or not the prior on t_sec was left open or if it was fixed to the time of injection t_{in j}, and the fourth column denotes the choice of the model when fitting the light curve. Finally, the last two columns show whether the eclipse was detected (how many standard deviations away from 0), and whether it was well measured (how many standard deviations away from f_{in j}). The red-yellow-green colour code highlights the significance of the detection and measurement for visual clarity.