Showing 1–20 of 56 results
/ Date/ Name
Nov 28, 2025ExoJAX Retrievals of VLT/CRIRES Spectra of Luhman 16AB: C/O Ratios and Systematic UncertaintiesMay 18, 2023Optical Alignment Method for the PRIME TelescopeJan 12, 2022OGLE-2016-BLG-1093Lb: A Sub-Jupiter-mass Spitzer Planet Located in Galactic BulgeMar 31, 2022KMT-2021-BLG-1077L: The fifth confirmed multiplanetary system detected by microlensingApr 9, 2022Systematic KMTNet Planetary Anomaly Search. V. Complete Sample of 2018 Prime-FieldJul 3, 2023KMT-2022-BLG-0475Lb and KMT-2022-BLG-1480Lb: Microlensing ice giants detected via non-caustic-crossing channelJan 8, 2024Systematic KMTNet Planetary Anomaly Search. XI. Complete Sample of 2016 Sub-Prime Field PlanetsApr 28, 2025Microlensing events indicate that super-Earth exoplanets are common in Jupiter-like orbitsMar 25, 2025Systematic Reanalysis of KMTNet Microlensing Events, Paper II: Two New Planets in Giant-Source EventsAug 20, 2025The Prime Focus Infrared Microlensing Experiment (PRIME): First ResultsJun 26, 2025KMT-2022-BLG-0086: Another binary-lens binary-source microlensing eventMay 16, 2022MOA-2019-BLG-008Lb: a new microlensing detection of an object at the planet/brown dwarf boundaryMay 21, 2022Four sub-Jovian-mass planets detected by high-cadence microlensing surveysJan 20, 2024MOA-2022-BLG-563Lb, KMT-2023-BLG-0469Lb, and KMT-2023-BLG-0735Lb: Three sub-Jovian-mass microlensing planetsApr 9, 2024OGLE-2018-BLG-0971, MOA-2023-BLG-065, and OGLE-2023-BLG-0136: Microlensing events with prominent orbital effectsSep 10, 2022Brown-dwarf companions in microlensing binaries detected during the 2016--2018 seasonsMay 11, 2023Probable brown dwarf companions detected in binary microlensing events during the 2018-2020 seasons of the KMTNet surveyNov 22, 2023KMT-2023-BLG-1431Lb: A New $q < 10^{-4}$ Microlensing Planet from a Subtle SignatureJun 15, 2024Four microlensing giant planets detected through signals produced by minor-image perturbationsNov 14, 2024KMT-2021-BLG-0284, KMT-2022-BLG-2480, and KMT-2024-BLG-0412: Three microlensing events involving two lens masses and two source stars