Gaia21efs: likely CV (dwarf nova?)
Tonny Vanmunster reported observations. The data
show 0.15 mag variations (flickering or part of
early superhumps?). The object is thus unlikely
a microlensing, but likely a CV. Spectroscopy is
encouraged.
OT J002656.6+284933 superhumps
(=CSS101212:002657+284933)
Sano-san and Tamas Tordai have reported observations.
0.3-mag superhumps are clearly present.
OT J002656.6+284933 superoutburst
(=CSS101212:002657+284933)
This object is known as an SU UMa star above
the period gap with multiple rebrightenings.
The last outburst was recorded in 2016.
https://ui.adsabs.harvard.edu/abs/2017PASJ...69L...4K/abstract
YYYYMMDD(UT) mag observer
20211013.6632 <159c (Yutaka Maeda)
20211014.6574 <167c (Yutaka Maeda)
20211015.6572 <165c (Yutaka Maeda)
20211017.6568 <158c (Yutaka Maeda)
20211023.5999 154:c (Yutaka Maeda)
20211025.5847 153cG (Yutaka Maeda)
20211026.5832 152:cG (Yutaka Maeda)
20211027.5983 153:cG (Yutaka Maeda)
OGLE-MC-DN-0008: new SU UMa-type dwarf nova
Josch Hambsch has reported observations on two nights.
The object shows 0.17-mag superhumps with a period
of 0.06056(8) d.
ASASSN-21tr: superhump period
Tonny Vanmunster, Tamas Tordai and Itoh-san have
reported observations. The superhump period since
Oct. 25 is 0.0666(2) d. The amplitude is still
small (0.06 mag) and they are most likely stage A
superhumps.
XM78HT: regular superhumps
The most recent data by Kyoto U. team on Oct. 26
detected clear ordinary superhumps. The superhumps
started growing on Oct. 25 (Vihorlat Obs. team).
The current period (stage A) is 0.05596(8) d.
IPHAS J184326.48+060800.9 (eclipsing polar) high state
http://gsaweb.ast.cam.ac.uk/alerts/alert/Gaia21ewn/
High state of this polar has not been seen
in the ZTF data. First time in recent years.
See [vsnet-chat 8874] (Sep. 22) about the nature of
this object.