ZTF22abteqxm: new WZ Sge-type dwarf nova
According to Itoh-san's observations on Nov. 18,
this object showed superhumps with a period of 0.0580(4) d
(single-night baseline). They were not very apparent
on Nov. 17 in Kyoto U. team observations.
An analysis of earlier data yielded a period of 0.05630(3) d
with an amplitude of 0.04 mag. These modulations appear
to be early superhumps. Observers are Kyoto U. team,
Itoh-san, Josch Hambsch and Tamas Tordai.