SIMBAD references

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 θ_E) and mass ratio are (s, q x 10³) = (1.81 ± 0.02, 1.24 ± 0.07) and (s, q x 10³) = (1.25 ± 0.03, 2.38 ± 0.08), respectively. From Bayesian analyses, we estimate the host and planet masses as (M_h,M_p)=(0.25_–0.13^+0.27M_☉,0.32_–0.17^+0.34M_J) and (M_h,M_p)=(0.54_–0.28^+0.33M_☉,1.34_–0.70^+0.82M_J), respectively. These planetary systems are located at a distance of 7.06_–1.15^+0.93kpc for OGLE-2018-BLG-0567 and 6.50_–1.75^+1.06kpc 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.