V375 UMa
Kiyota-san and Itoh-san reported observations.
There were only low-amplitude variations on Mar. 15 and 16.
Superhumps may have not yet developed.
TCP J06461075+2502415: most likely WZ Sge-type dwarf nova
Kiyota-san and Itoh-san have reported observations
(also some data from Magnus Larsson). The observations
show likely early superhumps with a period of 0.053(1) d
and an amplitude of 0.05 mag. The period was based on
a few cycles and will be updated as more data become
available.