%AHan, Cheongho%AUdalski, Andrzej%ALee, Chung-Uk%AKim, Doeon%AZhu, Wei%AAlbrow, Michael%AChung, Sun-Ju%AGould, Andrew%AHwang, Kyu-Ha%AJung, Youn%AKim, Hyoun-Woo%ARyu, Yoon-Hyun%AShin, In-Gu%AShvartzvald, Yossi%AYee, Jennifer%AZang, Weicheng%ACha, Sang-Mok%AKim, Dong-Jin%AKim, Seung-Lee%ALee, Dong-Joo%ALee, Yongseok%APark, Byeong-Gon%APogge, Richard%AKim, Chun-Hwey%AKim, Woong-Tae%AMróz, Przemek%ASzymański, Michał%ASkowron, Jan%APoleski, Radosław%ASoszyński, Igor%APietrukowicz, Paweł%AKozłowski, Szymon%ARybicki, Krzysztof%AIwanek, Patryk%AUlaczyk, Krzysztof%AWrona, Marcin%AGromadzki, Mariusz%ABuckley, David%ADong, Subo%ALuo, Ali%BJournal Name: Astronomy & Astrophysics; Journal Volume: 658 %D2022%I %JJournal Name: Astronomy & Astrophysics; Journal Volume: 658 %K %MOSTI ID: 10350595 %PMedium: X %TOGLE-2019-BLG-0468Lb,c: Two microlensing giant planets around a G-type star %XAims. With the aim of interpreting anomalous lensing events with no suggested models, we conducted a project of reinvestigating microlensing data collected in and before the 2019 season. In this work, we report a multi-planet system, OGLE-2019-BLG-0468L, that was found as a result of this project. Methods. The light curve of the lensing event OGLE-2019-BLG-0468, which consists of three distinctive anomaly features, could not be explained by the usual binary-lens or binary-source interpretations. We find a solution that explains all anomaly features with a triple-lens interpretation, in which the lens is composed of two planets and their host, making the lens the fourth multi-planet system securely found by microlensing. Results. The two planets have masses of ~3.4  M J and ~10.2  M J , and they are orbiting around a G-type star with a mass of ~0.9  M ⊙ and a distance of ~4.4 kpc. The host of the planets is most likely responsible for the light of the baseline object, although the possibility of the host being a companion to the baseline object cannot be ruled out. %0Journal Article