WASP-43 normalized light curves with best-fit models superimposed. For clarity a vertical offset was applied to the different LCs. The lower part of the diagram shows the best-fit residuals. Data are phase-folded according to the orbital period reported in Table 4 and the epochs of mid-transit reported in Table 3 . For each LC we report the telescope and the date of observation. In all cases a Johnson R filter was used.