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.