Showing 1–20 of 40 results
/ Date/ Name
Apr 24, 2025Energy partitioning between thermal and non-thermal electrons and ions in magnetotail reconnectionNov 28, 2022Energetic electron precipitation driven by electromagnetic ion cyclotron waves from ELFIN's low altitude perspectiveJun 18, 2021Direct Evidence for Magnetic Reflection of Heavy Ions from High Mach Number Collisionless ShocksNov 30, 2020In situ evidence of ion acceleration between consecutive reconnection jet frontsDec 24, 2019High-Resolution Near-Infrared Polarimetry and Sub-Millimeter Imaging of FS Tau A: Possible Streamers in Misaligned Circumbinary Disk SystemNov 25, 2019SUBARU Near-Infrared Imaging Polarimetry of Misaligned Disks Around The SR24 Hierarchical Triple SystemNov 19, 2018Multi-epoch Direct Imaging and Time-Variable Scattered Light Morphology of the HD 163296 Protoplanetary DiskAug 15, 2018Orbital characterization of GJ1108A system, and comparison of dynamical mass with model-derived mass for resolved binariesAug 8, 2017The Fundamental Stellar Parameters of FGK Stars in the SEEDS SurveyApr 19, 2017The Hyper Suprime-Cam SSP Survey: Overview and Survey DesignOct 4, 2016Radial decoupling of small and large dust grains in the transitional disk RX J1615.3-3255May 4, 2016Extreme Asymmetry in the Disk of V1247 OriMar 7, 2016High-Contrast Imaging of Intermediate-Mass Giants with Long-Term Radial Velocity TrendsJan 5, 2016Near-Infrared Imaging Polarimetry of LkCa 15: A Possible Warped Inner DiskJul 10, 2015Near-IR Polarized Scattered Light Imagery of the DoAr 28 Transitional DiskMay 19, 2015Detailed structure of the outer disk around HD 169142 with polarized light in H-bandMar 6, 2015Discovery of a Disk Gap Candidate at 20 AU in TW HydraeNov 10, 2014The Structure of Pre-transitional Protoplanetary Disks. II. Azimuthal Asymmetries, Different Radial Distributions of Large and Small Dust Grains in PDS~70Sep 4, 2014Surface Geometry of Protoplanetary Disks Inferred From Near-Infrared Imaging PolarimetryApr 21, 2014A Statistical Analysis of SEEDS and Other High-Contrast Exoplanet Surveys: Massive Planets or Low-Mass Brown Dwarfs?