Showing 1–20 of 45 results
/ Date/ Name
Sep 29, 2025Dynamical Architectures of S-type Transiting Planets in Binaries II: A Dichotomy in Orbital Alignment of Small Planets in Close Binary SystemsFeb 6, 2025Planet Masses, Radii, and Orbits from NASA's K2 MissionJan 10, 2025The TESS-Keck Survey XXIV: Outer Giants may be More Prevalent in the Presence of Inner Small PlanetsAug 14, 2024The $\sim$50-Myr-Old TOI-942c is Likely on an Aligned, Coplanar Orbit and Losing MassJul 30, 2024Obliquity Constraints for the Extremely Eccentric Sub-Saturn Kepler-1656 bMay 23, 2024The TESS-Keck Survey XX: 15 New TESS Planets and a Uniform RV Analysis of all Survey TargetsMay 21, 2024The TESS-Keck Survey. XXII. A sub-Neptune Orbiting TOI-1437Feb 12, 2024The TESS-Keck Survey. XII. A Dense 1.8 R$_\oplus$ Ultra-Short-Period Planet Possibly Clinging to a High-Mean-Molecular-Weight Atmosphere After the First GyrFeb 11, 2024The TESS-Keck Survey. XVIII. A sub-Neptune and spurious long-period signal in the TOI-1751 systemDec 4, 2023Validation of elemental and isotopic abundances in late-M spectral types with the benchmark HIP 55507 AB systemJun 30, 2023A VERITAS/Breakthrough Listen Search for Optical TechnosignaturesJun 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 StarsOct 31, 2022TESS Giants Transiting Giants III: An eccentric warm Jupiter supports a period-eccentricity relation for giant planets transiting evolved starsJun 28, 2022The TESS-Keck Survey. XIII. An Eccentric Hot Neptune with a Similar-Mass Outer Companion around TOI-1272Mar 31, 2022Kepler-1656b's Extreme Eccentricity: Signature of a Gentle GiantJan 11, 2022The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 day Orbit with the Automated Planet Finder TelescopeOct 11, 2021The TESS-Keck Survey. VI. Two Eccentric sub-Neptunes Orbiting HIP-97166Aug 11, 2021LkH$α$ 225 (V1318 Cyg) South in OutburstMay 18, 2021TKS X: Confirmation of TOI-1444b and a Comparative Analysis of the Ultra-short-period Planets with Hot Neptunes