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Characterizing a planet detected by microlensing is hard if the planetarysignal is weak or the lens-source relative trajectory is far from caustics.However, statistical analyses of planet demography must include those planetsto accurately determine occurrence rates. As part of a systematic modelingeffort in the context of a $>10$-year retrospective analysis of MOA's surveyobservations to build an extended MOA statistical sample, we analyze the lightcurve of the planetary microlensing event MOA-2014-BLG-472. This event providesweak constraints on the physical parameters of the lens, as a result of aplanetary anomaly occurring at low magnification in the light curve. We use aBayesian analysis to estimate the properties of the planet, based on a refinedGalactic model and the assumption that all Milky Way's stars have an equalplanet-hosting probability. We find that a lens consisting of a$1.9^{+2.2}_{-1.2}\,\mathrm{M}_\mathrm{J}$ giant planet orbiting a$0.31^{+0.36}_{-0.19}\,\mathrm{M}_\odot$ host at a projected separation of$0.75\pm0.24\,\mathrm{au}$ is consistent with the observations and is mostlikely, based on the Galactic priors. The lens most probably lies in theGalactic bulge, at $7.2^{+0.6}_{-1.7}\mathrm{kpc}$ from Earth. The accuratemeasurement of the measured planet-to-host star mass ratio will be included inthe next statistical analysis of cold planet demography detected bymicrolensing.

New Giant Planet beyond the Snow Line for an Extended MOA Exoplanet Microlens Sample