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MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals
by: Han, Cheongho, et al.
Published: (2025)
by: Han, Cheongho, et al.
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MOA-2022-BLG-563Lb, KMT-2023-BLG-0469Lb, and KMT-2023-BLG-0735Lb: Three sub-Jovian-mass microlensing planets
by: Han, Cheongho, et al.
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KMT-2023-BLG-1866Lb: Microlensing super-Earth around an M dwarf host
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by: Han, Cheongho, et al.
Published: (2024)
MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals
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KMT-2021-BLG-2609Lb and KMT-2022-BLG-0303Lb: Microlensing planets identified through signals produced by major-image perturbations
by: Han, Cheongho, et al.
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by: Han, Cheongho, et al.
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OGLE-2018-BLG-0971, MOA-2023-BLG-065, and OGLE-2023-BLG-0136: Microlensing events with prominent orbital effects
by: Han, Cheongho, et al.
Published: (2024)
by: Han, Cheongho, et al.
Published: (2024)
KMT-2022-BLG-0086: Another binary-lens binary-source microlensing event
by: Chung, Sun-Ju, et al.
Published: (2025)
by: Chung, Sun-Ju, et al.
Published: (2025)
KMT-2021-BLG-0284, KMT-2022-BLG-2480, and KMT-2024-BLG-0412: Three microlensing events involving two lens masses and two source stars
by: Han, Cheongho, et al.
Published: (2024)
by: Han, Cheongho, et al.
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KMT-2025-BLG-1616Lb: First Microlensing Bound Planet From DREAMS
by: Yang, Hongjing, et al.
Published: (2026)
by: Yang, Hongjing, et al.
Published: (2026)
KMT-2016-BLG-1337L: A Saturn-mass planet orbiting within a binary system of low-mass stars
by: Han, Cheongho, et al.
Published: (2026)
by: Han, Cheongho, et al.
Published: (2026)
KMT-2023-BLG-0416, KMT-2023-BLG-1454, KMT-2023-BLG-1642: Microlensing planets identified from partially covered signals
by: Han, Cheongho, et al.
Published: (2024)
by: Han, Cheongho, et al.
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OGLE-2015-BLG-1609Lb: Sub-jovian planet orbiting a low-mass stellar or brown dwarf host
by: Mróz, M. J., et al.
Published: (2024)
by: Mróz, M. J., et al.
Published: (2024)
The Microlensing Event Rate and Optical Depth from MOA-II 9 year Survey toward the Galactic Bulge
by: Nunota, Kansuke, et al.
Published: (2024)
by: Nunota, Kansuke, et al.
Published: (2024)
MOA-2020-BLG-135Lb: A New Neptune-class Planet for the Extended MOA-II Exoplanet Microlens Statistical Analysis
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Published: (2022)
by: Silva, Stela Ishitani, et al.
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OGLE-2023-BLG-0836L: The sixth microlensing planet in a binary stellar system
by: Han, Cheongho, et al.
Published: (2024)
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Mass Production of 2023 KMTNet Microlensing Planets. II: Two Planets and A Brown Dwarf
by: Li, Zhixing, et al.
Published: (2026)
by: Li, Zhixing, et al.
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Measurement of Dependence of Microlensing Planet Frequency on The Host Star Mass and Galactocentric Distance by using a Galactic Model
by: Nunota, Kansuke, et al.
Published: (2024)
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Analyses of anomalous lensing events detected from the UKIRT microlensing survey
by: Han, Cheongho, et al.
Published: (2025)
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Microlensing brown-dwarf companions in binaries detected during the 2022 and 2023 seasons
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Keck and Hubble Observations Show That MOA-2008-BLG-379Lb Is a Super-Jupiter Orbiting an M Dwarf
by: Bennett, David P., et al.
Published: (2023)
by: Bennett, David P., et al.
Published: (2023)
A Comprehensive Analysis of Three Microlensing Planet Candidates with the Planet/Binary Degeneracy
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"Industrial-Scale" Black Hole Selection without a Satellite
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Six microlensing planets detected via sub-day signals during the 2023 -- 2024 season
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Four binary microlenses with directly measured masses
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Mass Production of 2023 KMTNet Microlensing Planets. III: Three Planets from the Subprime Field
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Published: (2026)
by: Li, Hongyu, et al.
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Systematic Reanalysis of KMTNet Microlensing Events, Paper II: Two New Planets in Giant-Source Events
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Published: (2025)
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Systematic KMTNet Planetary Anomaly Search. XI. Complete Sample of 2016 Sub-Prime Field Planets
by: Shin, In-Gu, et al.
Published: (2024)
by: Shin, In-Gu, et al.
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Six binary brown dwarf candidates identified by microlensing
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Published: (2025)
by: Han, Cheongho, et al.
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OGLE-2015-BLG-0845L: A low-mass M dwarf from the microlensing parallax and xallarap effects
by: Hu, Zhecheng, et al.
Published: (2024)
by: Hu, Zhecheng, et al.
Published: (2024)
KMT-2024-BLG-0404L: A triple microlensing system consisting of a star, a brown dwarf, and a planet
by: Han, Cheongho, et al.
Published: (2025)
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Three Saturn-mass Microlensing Planets Identified through Signals from Peripheral-caustic Perturbations
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Candidate Microlensing Brown Dwarfs in Binary Lens Systems from the 2023--2025 Observing Seasons
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Engagement in Self‐Care Activities among Dementia Caregivers: A Content Analysis of Micro‐Longitudinal Digital Journal Data
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Four Giant Planets from 2024 KMTNet Microlensing Campaign
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On the Reparameterization Between Cartesian Position-Velocity Vectors and Orbital Elements in the Kepler Problem
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Image-Constrained Modeling with Hubble and Keck Images Reveals that OGLE-2012-BLG-0563Lb is a Jupiter-Mass planet Orbiting a K Dwarf
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KMT-2023-BLG-2669: Ninth Free-floating Planet Candidate with $θ_{\rm E}$ measurements
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Published: (2024)
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Four microlensing giant planets detected through signals produced by minor-image perturbations
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OGLE-2016-BLG-1195Lb: A Sub-Neptune Beyond the Snow Line of an M-dwarf Confirmed by Keck AO
by: Vandorou, Aikaterini, et al.
Published: (2023)
by: Vandorou, Aikaterini, et al.
Published: (2023)
Mass Production of 2023 KMTNet Microlensing Planets I: Low Mass Ratio
by: Ryu, Yoon-Hyun, et al.
Published: (2026)
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Similar Items
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MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals
by: Han, Cheongho, et al.
Published: (2025) -
MOA-2022-BLG-563Lb, KMT-2023-BLG-0469Lb, and KMT-2023-BLG-0735Lb: Three sub-Jovian-mass microlensing planets
by: Han, Cheongho, et al.
Published: (2024) -
KMT-2023-BLG-1866Lb: Microlensing super-Earth around an M dwarf host
by: Han, Cheongho, et al.
Published: (2024) -
MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals
by: Han, Cheongho, et al.
Published: (2025) -
KMT-2021-BLG-2609Lb and KMT-2022-BLG-0303Lb: Microlensing planets identified through signals produced by major-image perturbations
by: Han, Cheongho, et al.
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