Top panel: unbinned instrumental ﹩r﹩ band light curve of HATS-36 folded with at the period ﹩P=4.1752387﹩ days. The solid magenta line shows the best-fit transit model (see Section 3). Middle panel: a zoom-in on the transit; the dark blue filled points here show the light curve binned in phase using a bin-size of 0.002. Lower panel: the residuals to the best-fit model.