WX Cet started to show superhumps
According to the most recent observations by Josch Hambsch,
WX Cet started to show superhumps on Oct. 4 or 5.
Itoh-san obtained long time-series data starting from
the rising phase, but superhumps were not apparent
up to Oct. 3.
SDSS J001153.08-064739.1 rare bright outburst
Moriyama-san has pointed out that this object is
undergoing a rare bright outburst. The orbital period
is in the period gap and a superoutburst can be expected.
https://ui.adsabs.harvard.edu/abs/2014ApJ...790...28R/abstract
Using ZTF data, I obtained an orbital period
of 0.1002809(1) d. The phased light curve show clear
EW-like modulations with an amplitude of 0.25 mag.
YYYYMMDD(UT) mag observer
20220703.4593 17.813zg (Zwicky …
[View More]Transient Facility (Masci et al., 2019))
20220706.4376 17.765zg (Zwicky Transient Facility (Masci et al., 2019))
20220917.3159 17.539zg (ZTF Alert DC mag (Masci+ 2019))
20220929.2732 14.095zg (ZTF Alert DC mag (Masci+ 2019))
20221003.6523 13.10C (Masayuki Moriyama)
20221005.5858 13.51C (Masayuki Moriyama)
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ASASSN-22lx: new SU UMa-type dwarf nova
Josch Hambsch and Berto Monard have reported observations.
This object started to show superhumps on Oct. 4.
The current period is 0.0564(5) d.
ASASSN-22lk: superhump period
Period = 0.05584(2) d, amplitude 0.12 mag (after Sep. 27).
My analysis suggests that early superhumps were below
the detection limit.
Observers: Kyoto U. team, Itoh-san, Tonny Vanmunster.
TCP J23580961+5502508: updated period of early superhumps
Period = 0.05940(1) d. Mean amplitude 0.15 mag.
Observers: Kyoto U. team, Itoh-san, Osaka Kyoiku U. team,
Kiyota-san, Tamas Tordai, Sano-san, Josch Hambsch