Showing 21–40 of 112 results
/ Date/ Name
May 19, 2023EUV fine structure and variability associated with coronal rain revealed by Solar Orbiter/EUI HRIEUV and SPICEMay 9, 2023Coronal Heating as Determined by the Solar Flare Frequency Distribution Obtained by Aggregating Case StudiesJan 13, 2023First Perihelion of EUI on the Solar Orbiter missionDec 19, 2022I2D2: Inductive Knowledge Distillation with NeuroLogic and Self-ImitationSep 29, 2022An old warm Jupiter orbiting the metal-poor G-dwarf TOI-5542Sep 18, 2022Distribution inference risks: Identifying and mitigating sources of leakageApr 19, 2022ParticLS: Object-oriented software for discrete element methods and peridynamicsMar 4, 2022A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino PhysicsOct 25, 2021The young HD 73583 (TOI-560) planetary system: Two 10-M$_\oplus$ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarfJul 24, 2021Anomalous nematic-to-stripe phase transition driven by in-plane magnetic fieldsMay 13, 2021Interaction Effects and Viscous Magneto-Transport in a Strongly Correlated 2D Hole SystemApr 30, 2021TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrAJan 12, 2021A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113Dec 25, 2020Incipient Formation of the Reentrant Insulating Phase in a Dilute 2D Hole System with Strong InteractionsOct 16, 2020Reflective Decoding: Beyond Unidirectional Generation with Off-the-Shelf Language ModelsOct 12, 2020Back to the Future: Unsupervised Backprop-based Decoding for Counterfactual and Abductive Commonsense ReasoningOct 8, 2020Statistical Signatures of Nanoflare Activity. II. A Nanoflare Explanation for Periodic Brightenings in Flare Stars observed by NGTSSep 23, 2020Three-Dimensional Reconstructions of Coronal Wave Surfaces Using a New Mask-Fitting MethodJul 15, 2020Search for $hep$ solar neutrinos and the diffuse supernova neutrino background using all three phases of the Sudbury Neutrino ObservatoryApr 21, 2020Long-term Evolution of the Solar Corona Using PROBA2 Data