Fig. 2
Secondary-eclipse light curves of WASP-46b as observed with GROND in the g′r′i′z′ bands. Left panel: light curves that are normalized by the reference stars. Middle panel: baseline-corrected light curves that are binned every 10 min for display purpose. Right panel: best-fit light-curve residuals that are binned every 10 min. All the best-fit models are indicated by solid lines.
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