ASASSN-22jz: new WZ Sge-type dwarf nova
Berto Monard has reported observations on two nights.
The object was fading rather rapidly (0.3 mag/d),
probably in viscous fading phase.
Although there were much irregularity, I could detect
a period of 0.05404(4) d (double wave, 0.035 mag).
Although the profile is not very typical for early superhumps,
the period appears to be real based on the appearance of
one-day aliases. The rather unusual profile of
early superhumps a result of their low amplitude and
overlapping irregularity. Considering the outburst
amplitude and peak M_V, this object can be identified
to be a WZ Sge star.