Positive superhumps in V425 Cas
Using TESS data, I obtained the orbital period
of 0.14899(3) d (amplitude 0.05 mag).
Positive superhumps with a mean period of
0.16505(4) d (0.06 mag) were also detected.
V1363 Cyg: orbital period
Using TESS data, I obtained an orbital period of
0.7984(2) d. The light curve suggests shallow eclipses
with 0.17 mag primary and 0.09 mag secondary superimposed
on reflection effect.
The value (20-40 hr) suggested in
https://ui.adsabs.harvard.edu/abs/2022arXiv220205699S/abstract
is somewhat an overestimate.
MGAB-V1183: R
This object is R (not R+E:). P=0.03497920(3) d from
the ZTF data. Eclipse-like events in the older ZTF data
were noises (no periodicity). No such events in the recent
data.
NADA-V123: R
Using TESS data, I obtained a very clear sinusoidal
light curve with an amplitude of 0.15 mag.
This object is not IBWD: but R. Detached WD+SD binaries
below the period minimum are rare and this object needs
to be studied in more detail.