[vsnet-alert 20334] GS Cet: new WZ Sge-type dwarf nova

[Taichi Kato]

GS Cet: new WZ Sge-type dwarf nova

   Kiyota-san has reported time-resolved photometry.
The data show the presence of early superhumps
with an amplitude of 0.07 mag.  The period
(0.057 d) is slightly different from the published
orbital period, but the difference may have been
due to the short baseline and air-mass effect which
has not yet been well determined.
Further observations will clarify the period.