  We report the discovery and the analysis of the short timescale binary-lens
microlensing event, MOA-2015-BLG-337. The lens system could be a planetary
system with a very low mass host, around the brown dwarf/planetary mass
boundary, or a brown dwarf binary. We found two competing models that explain
the observed light curves with companion/host mass ratios of q~0.01 and ~0.17,
respectively. From the measurement of finite source effects in the best-fit
planetary model, we find a relatively small angular Einstein radius of theta_E
~ 0.03 mas which favors a low mass lens. We conduct a Bayesian analysis to
obtain the probability distribution of the lens properties. The results for the
planetary models strongly depend on the minimum mass, M_min, in the assumed
mass function. In summary, there are two solutions of the lens system: (1) a
brown dwarf/planetary mass boundary object orbited by a super-Neptune (the
planetary model with M_min=0.001 M_sun) and (2) a brown dwarf binary (the
binary model). If the planetary models is correct, this system can be one of a
new class of planetary system, having a low host mass and also a planetary mass
ratio (q <0.03) between the host and its companion. The discovery of the event
is important for the study of planetary formation in very low mass objects. In
addition, it is important to consider all viable solutions in these kinds of
ambiguous events in order for the future comprehensive statistical analyses of
planetary/binary microlensing events.
