Fig. 2

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Example of a synthetic light curve generated with Pandora. The shown system (system ID: simu 21) consists of a Jupiter-sized planet with a 30-day orbital period and a 3 R⊕ exomoon on a 1-day orbital period. The simulation assumes a target star with 6 ≤ mV ≤ 10.5 and white Gaussian noise of 138 ppm per 2-minute cadence. The plot displays the flux variation during one planetary transit event, clearly showing the modulation induced by the moon’s orbit.
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