Fig. 5
Phase-folded IRAC 8-μm HD 189733b’s photometry binned per 1 min and corrected for the systematics (black dots) with their 1σ error bars (red triangles) and the best-fitting eclipse models superimposed. Left: phase-folded transits. Right: phase curve and phase-folded occultations that show the benefit of using non-uniform brightness model.
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