ASASSN-22cw: most likely new WZ Sge-type dwarf nova
Berto Monard has reported observations. Two cycles
of variations were recorded. The period was 0.0528(7) d
and a full amplitude of 0.08 mag. The profile is
doubly humped with the second one brighter and this
suggests that the variation early superhumps.
Note that the period may be shorter than 0.05332 d
in GW Lib. Further observations are needed to
confirm and then update the period.