Fig. 2

Occultation light curves of WASP-43b as observed with GROND. In each panel, shown
from top to bottom are the occultation light curves of
g′r′i′z′JHK.
Left panel: light curves that are normalized by the reference
stars. Middle panel: baseline-corrected light curves that are
binned every 8 min for display purpose (see Sect. 3.1 for baseline correction). Right panels: best-fit
light-curve residuals, also binned every 8 min. Best-fit models for all panels are
overlaid in solid or dashed lines. The occultation depth is detected in the
K-band (0.197 ± 0.042%) and
marginally detected in the i′-band (0.037
%).
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