Gaia16ahn possible superoutburst
Likely SU UMa star from ZTF data. Likely superoutburst
in 2022 Julu-Aug. The current outburst is fainter.
YYYYMMDD(UT) mag observer
20230128.1410 18.088zg (ZTF Alert DC mag (Masci+ 2019))
20230128.2015 17.611zr (ZTF Alert DC mag (Masci+ 2019))
20230202.1541 16.656zg (ZTF Alert DC mag (Masci+ 2019))
CRTSJ141002.2-124809 possible superoutburst
Likely SU UMa star from ZTF data.
YYYYMMDD(UT) mag observer
20221224.5278 19.951zg (ZTF Alert DC mag (Masci+ 2019))
20230124.5403 20.437zg (ZTF Alert DC mag (Masci+ 2019))
20230202.4168 16.039zr (ZTF Alert DC mag (Masci+ 2019))
20230202.5385 16.030zg (ZTF Alert DC mag (Masci+ 2019))
Re: UGWZ star CRTSJ174033.4+414756 outburst!
> I didn't realize the classification had changed. I will change my list
> immediately.
No special need. This object indeed underwent a WZ Sge-type
superoutburst in 2013.
PNVJ06245297+0208207: fading from superoutburst plateau
The object started fading rather rapidly on Jan. 31
(Itoh-san, Kiyota-san and Kyoto U. team).
The object reached about 15.5 mag on Feb. 1 (Itoh-san).
The superhump period during the superoutburst plateau
(up to Jan. 30) was 0.033372(5) d. Observers were
Kyoto U. team, Itoh-san, Kiyota-san, Crimean Astrophys.
Obs. team and Josch Hambsch).
This may be shorter than the orbital period
(see Kato 2022 arXiv:2201.02945).
The evolution of the outburst in this system is very
similar to SDSS J090221.35+381941.9 and it would brighten
again to a plateau phase. Have a look at the paper.
https://ui.adsabs.harvard.edu/abs/2014PASJ...66L...7K/abstract
Continued observations are requested.