Z Cam: oscillations before the termination of standstill
It would be worth noting that there were low-amplitude
oscillations since 2022 Oct., but without gradual brightening
seen in IW And stars. The disk apparently started becoming
thermally unstable before the termination of the standstill.
Oscillations were also seen for a month after entering
this standstill (2022 Apr.).
MASTER OT J021216.01+461154.5: no superhumps
Tonny Vanmunster and Tamas Tordai reported observations
on two nights. No superhumps were detected (at least as of
now).
CS Ind: observations on Jan. 4
Observations by Filipp Romanov obtained a rather flat
light curve (but only for 1 hr and it would be difficult
to exclude the presence of superhumps).
PNVJ06245297+0208207: no apparent superhumps yet
Tamas Tordai has reported observations. No large-amplitude
superhumps were present and this object is likely a helium
WZ Sge star with a low inclination.
Standstill in CR Boo
Using ATLAS forced photometry (Tonry et al. 2018;
Shingles et al. 2021) and observations reported to VSNET,
I found that CR Boo was almost constant between 2022 May and
early July. A faint state without a dwarf nova outburst
(around 17 mag) followed. The former appears to be
a true standstill without low-amplitude oscillations.
The latter may have reflected a lower mass-transfer rate,
but the duration was too short to be recognized as
a VY Scl-type fading episode. …
[View More]The object currently appears
to show dwarf nova outbursts.
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Very low state of AG Aps
Accoring to ATLAS forced photometry (Tonry et al. 2018;
Shingles et al. 2021), this object was near the limit of
detection (near 20.0 mag) in 2022. Outbursts were also
present, but very faint (17 mag).