We present the analysis of a planetary microlensing event OGLE-2019-BLG-0362 with a shortduration anomaly (∼0.4 days) near the peak of the light curve, which is caused by the resonant caustic. The event has a severe degeneracy with Δχ2 = 0.9 between the close and the wide binary lens models both with planet-host mass ratio q ≃ 0.007. We measure the angular Einstein radius but not the microlens parallax, and thus we perform a Bayesian analysis to estimate the physical parameters of the lens. We find that the OGLE-2019-BLG-0362L system is a super-Jovian-mass planet Mp = 3.26+0.83 −0.58 MJ orbiting an M dwarf Mh = 0.42+0.34 −0.23 M⊙ at a distance DL = 5.83+1.04 −1.55 kpc. The projected star-planet separation is a⊥ = 2.18+0.58 −0.72 AU, which indicates that the planet lies beyond the snow line of the host star.

The present study is aimed at determining how teaching and learning in Japanese translation/interpretation classes are linked to the modality relationships among hearsay markers, which are schematized after dividing the difference of pragmatics in the three following relationships: information and speaker, information and listener, and speaker and listener. Information about seven Japanese hearsay markers was collected through a questionnaire over native Japanese speakers. The findings revealed that people, first, chose [youda] and [toiukotoda] usually as the hearsay expressions, considering the relationship between information and speaker. Second, people divided [tonokotoda] into two relationships between information and speaker, or between information and listener. The responses about [souda] were split considering the relationship between information and speaker and speaker and listener. [Rashi] and [toka] were chosen the most, considering the relationship between information and listener, and there was a relatively large number of [toiu(utte)].