Fig. 2
Panels from top to bottom: (1) raw flux of WASP-127 (black line) and the reference star (red line) obtained with ALFOSC at NOT; (2) relative flux between the WASP-127 and the reference star (black dots) and the best-fitting combined model (red line); (3) same as in panel 2, but detrended; (4) best-fitting light-curve residuals.
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