ASASSN-22gx: new SU UMa-type dwarf nova
According to observations by Berto Monard on May 21-22,
superhumps with a period of 0.0584(2) d and an amplitude
of 0.19 mag were detected. Earlier observations on
May 14 and 15 by Josch Hambsch did not detected apparent
modulations.
XM116HT: period of early superhumps
Itoh-san, Tamas Tordai, Stephen Brincat, Tonny Vanmunster
and Vihorlat Observatory team have reported observations.
The period of early superhumps is 0.055839(9) d.
The variation is still prominent.
ZTF J181732.64+101954.5: ER UMa + Z Cam + IW And
From ZTF data. Supercycle about 56 d before 2020 May.
Then long standstill. ER UMa state e.g. 2019 July-Sep.
(normal outbursts + superoutburst).
In 2019 Mar.-June, two superoutbursts occurred
directly from a standstill (like NY Ser), but with
the same supercycle. Superhumps with a period of
0.08881(4) d (0.13 mag) were detected during
the 2019 June-July superoutburst.
IW And state (dip following superoutburst) was recorded
in 2018 Mar.-July.
XM116HT = TCP J14225968+4122545: WZ Sge-type star with prominent early superhumps
Tamas Tordai has reported observations. The object
shows double-wave 0.3-mag early superhumps.
The period is still somewhat uncertain (0.0557-0.0571 d).
Bright WZ Sge stars with large-amplitude early superhumps
are rare and observations are encouraged.