Top panel: Magellan light curve of J1650 phased on the photometric period of ﹩P=0.3205﹩ days. Middle panel: Phased light curve smoothed using 20 bins in phase, along with two representative ellipsoidal model fits (see Table 2 for model parameters). The solid line shows a model with an accretion that dominates the light (model A in Table 2), and the dot‐dashed line shows a model with no accretion disk (model B in Table 2). Bottom panel: Magellan light curve folded using the period of ﹩P=0.212﹩ days reported by SF02.