RZ LMi: possible orbital period
Using TESS data in 2020, I detected a period of
0.058005(8) d (amp. 0.02 mag). This value is close to
what was derived in Kato et al. (2016) PASJ 68, 107.
This result seems to strengthen the idea that the core
of the secondary in RZ LMi is evolved, as suggested
in Kato et al. (2016). This period was not very
apparent in TESS data in 2022.