ASASSN-22bs: new SU UMa (likely WZ Sge) star

According to the most recent data by Josch Hambsch, ordinary superhumps appeared on Feb. 16. The current period is about 0.06 d (amplitude 0.25 mag). Considering the relatively long waiting time (8 d), this object is likely a borderline WZ Sge/SU UMa system.