ASASSN-22ng: most likely SU UMa star fading from superoutburst
Josch Hambsch and Itoh-san have reported observations.
The object showed a typical SU UMa-type superoutburst
followed by rapid fading on Nov. 15.
Although some observations showed likely superhumps,
the period has not been reliably determined due to
short observations or poor S/N. Likely around 0.07 d
from observations on Nov. 4. The object is almost
certainly an SU UMa star and observations in better condition
during a future superoutburst are very much desirable.