We present the analyses of two microlensing events, OGLE-2018-BLG-0567 and OGLE-2018-BLG-0962. In both events, the short-lasting anomalies were densely and continuously covered by two high-cadence surveys. The light-curve modeling indicates that the anomalies are generated by source crossings over the planetary caustics induced by planetary companions to the hosts. The estimated planet/host separation (scaled to the angular Einstein radius θE) and mass ratio are (s,q)=(1.81,1.24×10−3) and (s,q)=(1.25,2.38×10−3), respectively. From Bayesian analyses, we estimate the host and planet masses as (Mh,Mp)=(0.24−0.13+0.16M⊙,0.32−0.16+0.34MJ) and (Mh,Mp)=(0.55−0.29+0.32M⊙,1.37−0.72+0.80MJ), respectively. These planetary systems are located at a distance of 7.07−1.15+0.93kpc for OGLE-2018-BLG-0567 and 6.47−1.73+1.04kpc for OGLE-2018-BLG-0962, suggesting that they are likely to be near the Galactic bulge. The two events prove the capability of current high-cadence surveys for finding planets through the planetary-caustic channel. We find that most published planetary-caustic planets are found in Hollywood events in which the source size strongly contributes to the anomaly cross section relative to the size of the caustic.