The original SPOC light curve and the light curve with masked outlying points for HD 295290 (top) and the corresponding detrended light curve with the identified flares (bottom). Because Z.-L. Tu et al. (2020) provided the times for the flares they identified, the peak times of their flares are also included in the bottom plot. Our flare-identification framework identified 14 flares for HD 295290 compared to Z.-L. Tu et al.’s (2020) eight flares and L. Doyle et al.’s (2020) 16 flares. Many of the flares we detected that were not reported by Z.-L. Tu et al. (2020) may have been excluded from their analysis because they did not qualify as superflares based on their energy calculations.