Left: Phased V‐band light curves of ST LMi from four nights of observing run A, as marked in Fig. 1 (bottom). Note the maxima near phase 0.8. Filled circles are data from the second of two adjacent orbital cycles. Right: Phased V‐band light curves of ST LMi from three nights of observing run B and one night of observing run C, as marked in Fig. 1 (bottom). Note the absence of a maximum near phase 0.8.