Showing 1–20 of 20 results
/ Date/ Name
Feb 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 PlanetsMay 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 GyrJun 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 StarsMar 9, 2023Light Curves and Colors of the Ejecta from Dimorphos after the DART ImpactNov 3, 2022A 16 Hour Transit of Kepler-167 e Observed by the Ground-based Unistellar Telescope NetworkOct 5, 2022A Catalog of Habitable Zone ExoplanetsJun 28, 2022The TESS-Keck Survey. XIII. An Eccentric Hot Neptune with a Similar-Mass Outer Companion around TOI-1272Mar 10, 2022The Lick Observatory Supernova Search follow-up program: photometry data release of 70 stripped-envelope supernovaeJan 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-97166Jul 28, 2021Asteroseismology of iota Draconis and Discovery of an Additional Long-Period CompanionMay 18, 2021TKS X: Confirmation of TOI-1444b and a Comparative Analysis of the Ultra-short-period Planets with Hot NeptunesDec 9, 2020Speckle Imaging Characterization of Radial Velocity Exoplanet SystemsSep 7, 2020The TESS-Keck Survey II: An Ultra-Short Period Rocky Planet and its Siblings Transiting the Galactic Thick-Disk Star TOI-561Jun 21, 2019A super-Earth and sub-Neptune transiting the late-type M dwarf LP 791-18Sep 12, 2016Long-term, Multiwavelength Light Curves of Ultra-cool Dwarfs: I. An Interplay of Starspots & Clouds Likely Drive the Variability of the L3.5 dwarf 2MASS 0036+18