Showing 1–20 of 79 results
/ Date/ Name
Oct 3, 2021Mysterious Dust-emitting Object Orbiting TIC 400799224Feb 19, 2024Short-Period Variables in TESS Full-Frame Image Light Curves Identified via Convolutional Neural NetworksJan 21, 2025Pioneering High-Speed Pulsar Parameter Estimation Using Convolutional Neural NetworksFeb 16, 2026Accelerating Posterior Inference from Pulsar Light Curves via Learned Latent Representations and Local Simulator-Guided OptimizationApr 21, 2026The swept-back multipolar magnetic field of neutron stars: Application to NICER MSP J0030+0451Oct 5, 2022MOA-2020-BLG-208Lb: Cool Sub-Saturn Planet Within Predicted DesertJan 26, 2021Identifying Planetary Transit Candidates in TESS Full-Frame Image Light Curves via Convolutional Neural NetworksNov 27, 2018Generalizing semi-supervised generative adversarial networks to regression using feature contrastingJan 31, 2019Improving Dense Crowd Counting Convolutional Neural Networks using Inverse k-Nearest Neighbor Maps and Multiscale UpsamplingJan 12, 2021OGLE-2019-BLG-0960Lb: The Smallest Microlensing PlanetJan 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 EventsJun 26, 2025KMT-2022-BLG-0086: Another binary-lens binary-source microlensing eventMar 15, 2023Free-Floating planet Mass Function from MOA-II 9-year survey towards the Galactic BulgeSep 3, 2023KMT-2021-BLG-1547Lb: Giant microlensing planet detected through a signal deformed by source binarity