ASASSN-22as: new SU UMa (or even WZ Sge?) star in the period gap
Tonny Vanmunster and Tamas Tordai have reported
observations. I could find a period of 0.09974(9) d
(full amplitude of 0.10 mag). The profile resembles
that of early superhumps (doubly peaked, sharp minimum)
rather than ordinary superhumps. It is also possible
that these superhumps are stage A superhumps.
If this is indeed a WZ Sge star, it is very unusual.
Further observations are needed to follow the development
of these superhumps.