Showing 21–40 of 100 results
/ Date/ Name
Jun 28, 2023A close-in giant planet escapes engulfment by its starOct 11, 2021The TESS-Keck Survey. VI. Two Eccentric sub-Neptunes Orbiting HIP-97166Aug 4, 2021TESS-Keck Survey IX: Masses of Three Sub-Neptunes Orbiting HD 191939 and the Discovery of a Warm Jovian Plus a Distant Sub-Stellar CompanionMay 12, 2021A Deep Polarimetric Study of the Asymmetrical Debris Disk HD 106906Feb 15, 2022Revisiting the Full Sets of Orbital Parameters for the XO-3 System: No evidence for Temporal Variation of the Spin-Orbit AngleJan 11, 2022The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 day Orbit with the Automated Planet Finder TelescopeJun 28, 2023The TESS-Keck Survey. XVI. Mass Measurements for 12 Planets in Eight SystemsJun 1, 2023The TESS-Keck Survey. XV. Precise Properties of 108 TESS Planets and Their Host StarsFeb 12, 2024The TESS-Keck Survey. XII. A Dense 1.8 R$_\oplus$ Ultra-Short-Period Planet Possibly Clinging to a High-Mean-Molecular-Weight Atmosphere After the First GyrFeb 20, 2024A Tale of Two Peas-In-A-Pod: The Kepler-323 and Kepler-104 SystemsMay 22, 2023The Spin-Orbit Misalignment of TOI-1842b: The First Measurement of the Rossiter-McLaughlin Effect for a Warm Sub-Saturn around a Massive StarMay 23, 2024The TESS-Keck Survey XX: 15 New TESS Planets and a Uniform RV Analysis of all Survey TargetsApr 9, 2024Evidence for Primordial Alignment: Insights from Stellar Obliquity Measurements for Compact Sub-Saturn SystemsJul 31, 2024TESS Giants Transiting Giants. VI. Newly Discovered Hot Jupiters Provide Evidence for Efficient Obliquity Damping after the Main SequenceSep 12, 2024HD 222237 b: a long period super-Jupiter around a nearby star revealed by radial-velocity and Hipparcos-Gaia astrometryJun 10, 2025JWST Coronagraphic Images of 14 Her c: a Cold Giant Planet in a Dynamically Hot, Multi-planet SystemDec 19, 2025Double Hot Jupiter Formation through Mirrored ZLK Migration in Binary Star Systems: The Case of WASP-94Sep 16, 2024SPORES-HWO. II. Companion Mass Limits and Updated Planet Properties for 120 Future Exoplanet Imaging Targets from 35 yr of Precise Doppler MonitoringDec 1, 2025The Astrometric Resoeccentric Degeneracy: Eccentric Single Planets Mimic 2:1 Resonant Planet Pairs in AstrometryJul 27, 2022Chemical Abundances for 25 JWST Exoplanet Host Stars with KeckSpec