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We present the analyses of two microlensing events, OGLE-2018-BLG-0567 andOGLE-2018-BLG-0962. In both events, the short-lasting anomalies were denselyand continuously covered by two high-cadence surveys. The light-curve modelingindicates that the anomalies are generated by source crossings over theplanetary caustics induced by planetary companions to the hosts. The estimatedplanet/host separation (scaled to the angular Einstein radius $\theta_{\rm E}$)and mass ratio are $(s, q) = (1.81, 1.24\times10^{-3})$ and $(s, q) = (1.25,2.38\times10^{-3})$, respectively. From Bayesian analyses, we estimate the hostand planet masses as $(M_{\rm h}, M_{\rm p}) =(0.24_{-0.13}^{+0.16}\,M_{\odot}, 0.32_{-0.16}^{+0.34}\,M_{\rm J})$ and$(M_{\rm h}, M_{\rm p}) = (0.55_{-0.29}^{+0.32}\,M_{\odot},1.37_{-0.72}^{+0.80}\,M_{\rm J})$, respectively. These planetary systems arelocated at a distance of $7.07_{-1.15}^{+0.93}\,{\rm kpc}$ forOGLE-2018-BLG-0567 and $6.47_{-1.73}^{+1.04}\,{\rm kpc}$ forOGLE-2018-BLG-0962, suggesting that they are likely to be near the Galacticbulge. The two events prove the capability of current high-cadence surveys forfinding planets through the planetary-caustic channel. We find that mostpublished planetary-caustic planets are found in Hollywood events in which thesource size strongly contributes to the anomaly cross section relative to thesize of the caustic.

OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: Two Microlensing Planets through Planetary-Caustic Channel