ASASSN-13bz: SU UMa star (or even WZ Sge)
Itoh-san detected superhumps on Dec. 3 (amplitude 0.12 mag).
The period from single-night baseline is 0.059(1) d.
I suspected this object to be an SS Cyg star based on
the initial fading rate (0.2-0.4 mag/d) and the lack of
superhumps, but this may have been a viscous decay phase
of a WZ Sge star (considering the rarity of outbursts).
Early superhumps may have not been present simply based on
a low inclination.
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