Phased V‐band light curves of ST LMi from 1990–2005 RoboScope data. The data consist of a single point each clear night, at a random orbital phase. Top: High‐state light curve showing a maximum near phase 0.8. Bottom: Low‐state light curve, perhaps showing a weak maximum near phase 0.8. The occasional brightward excursions are likely artifacts due to cosmic rays.