We present the analysis of three more planets from the KMTNet 2021 microlensing season. KMT-2021-BLG-0119Lb is a ~6M_Jup_ planet orbiting an early M-dwarf or a K-dwarf, KMT-2021-BLG-0192Lb is a ~2M_Nep_ planet orbiting an M-dwarf, and KMT-2021-BLG-2294Lb is a ~1.25M_Nep_ planet orbiting a very-low-mass M-dwarf or a brown dwarf. These by-eye planet detections provide an important comparison sample to the sample selected with the AnomalyFinder algorithm, and in particular, KMT-2021-BLG-2294 is a case of a planet detected by eye but not by algorithm. KMT-2021-BLG-2294Lb is part of a population of microlensing planets around very-low-mass host stars that spans the full range of planet masses, in contrast to the planet population at <~0.1au, which shows a strong preference for small planets.
Cone search capability for table J/AJ/165/8/table1 (Observations of 2021 planetary events)