ASASSN-22mr: start of long rebrightening
According to the data by Josch Hambsch, this object
experienced a dip from Oct. 30 to Nov. 1, then
rebrightened. The rebrightening appears to be a long one
such as in WZ Sge.
MGAB-V672 possible superoutburst
Type from ZTF data. Short supercycle (100-200 d)
and another superoutburst is due.
YYYYMMDD(UT) mag observer
20221030.4250 16.524zg (ZTF Alert DC mag (Masci+ 2019))
20221030.4791 16.438zr (ZTF Alert DC mag (Masci+ 2019))
TCP J06382808-0844347: new SU UMa-type dwarf nova
Itoh-san (and some from Josch Hambsch) reported
observations. This object is an SU UMa star with
a superhump period of 0.05457(2) d (mean amplitude
0.07 mag). A small degree of ambiguity about
one-day aliases remains.