TESS and CASLEO eclipse light curves of MML 48 compared to best fit model. Left: Primary-eclipse TESS light curve acquired during Sectors 11 (top), 38 (middle), and 65 (bottom). Overplotted is the PHOEBE best fit model in the I-band filter with a third light contamination (of 0.077 in units of total light for Sector 11, 0.064 for 38, and 0.091 for 65), and it is shown by the continuous red line. The individual data point photometric uncertainties are represented by the length of the vertical lines. Center: Secondary-eclipse TESS light curve compared to the best fit model. The TESS light curves are plotted on the same scale for comparison. Right: CASLEO light curves in VRI passbands (from top to bottom) of the MML 48 primary eclipse.