Showing 1–20 of 22 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 PlanetsJul 30, 2024Obliquity Constraints for the Extremely Eccentric Sub-Saturn Kepler-1656 bJun 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 StarsApr 10, 2023The James Webb Space Telescope MissionSep 30, 2022Retrieving C and O Abundance of HR 8799 c by Combining High- and Low-Resolution DataJun 28, 2022The TESS-Keck Survey. XIII. An Eccentric Hot Neptune with a Similar-Mass Outer Companion around TOI-1272Feb 5, 2022Retrieving the C and O Abundances of HR 7672~AB: a Solar-Type Primary Star with a Benchmark Brown DwarfJan 30, 2022NEID Rossiter-McLaughlin Measurement of TOI-1268b: A Young Warm Saturn Aligned with Its Cool Host StarJan 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 14, 2021Detection and Bulk Properties of the HR 8799 Planets with High Resolution SpectroscopyMay 18, 2021TKS X: Confirmation of TOI-1444b and a Comparative Analysis of the Ultra-short-period Planets with Hot NeptunesSep 7, 2020The TESS-Keck Survey II: An Ultra-Short Period Rocky Planet and its Siblings Transiting the Galactic Thick-Disk Star TOI-561Apr 21, 2020The multi-planet system TOI-421 -- A warm Neptune and a super puffy mini-Neptune transiting a G9 V star in a visual binaryFeb 1, 2019Stellar Spectroscopy in the Near-infrared with a Laser Frequency CombJun 8, 2014Earthshine on a Young Moon: Explaining the Lunar Farside HighlandsJul 29, 2013The Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution ExperimentJun 13, 2013A Cautionary Tale: MARVELS Brown Dwarf Candidate Reveals Itself To Be A Very Long Period, Highly Eccentric Spectroscopic Stellar Binary