Three anomalous microlensing events are re-modeled as binary-lens binary-source (2L2S) systems that resolve prior residuals, with source stars identified as G8V/M3V, G8V/K2V, and G6V/G8V pairs and lenses inferred as low-mass binaries via Bayesian methods.
Monthly Notices of the Royal Astronomical Society , volume =
3 Pith papers cite this work. Polarity classification is still indexing.
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Three new planets detected via 2023 KMTNet microlensing with mass ratios log q ~ -1.9, -2.0, -2.6; overall 2023 sample of 25 planets matches prior mass-ratio distribution.
Derived reliable rotation periods for 96 asteroids (84 new) from 2018 KMTNet data in one square degree field, projecting >5500 periods from full ~12 deg² dataset.
citing papers explorer
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Four-Body Gravitational Microlensing Events Involving Both a Binary Lens and a Binary Source
Three anomalous microlensing events are re-modeled as binary-lens binary-source (2L2S) systems that resolve prior residuals, with source stars identified as G8V/M3V, G8V/K2V, and G6V/G8V pairs and lenses inferred as low-mass binaries via Bayesian methods.
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Mass Production of 2023 KMTNet Microlensing Planets. III: Three Planets from the Subprime Field
Three new planets detected via 2023 KMTNet microlensing with mass ratios log q ~ -1.9, -2.0, -2.6; overall 2023 sample of 25 planets matches prior mass-ratio distribution.
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Measuring Asteroid Rotation Periods Using the KMTNet Bulge Survey Data
Derived reliable rotation periods for 96 asteroids (84 new) from 2018 KMTNet data in one square degree field, projecting >5500 periods from full ~12 deg² dataset.