Showing 1–20 of 24 results
/ Date/ Name
Feb 19, 2026Possible stratospheric emission in the warm Neptune GJ 436 b from high-resolution spectroscopyJan 9, 2026Distinct Rotational Evolution of Giant Planets and Brown Dwarf CompanionsNov 24, 2025Chemical and Isotopic Homogeneity Between the L Dwarf CD-35 2722 B and its Early M Host StarSep 29, 2025Dynamical Architectures of S-type Transiting Planets in Binaries II: A Dichotomy in Orbital Alignment of Small Planets in Close Binary SystemsMar 3, 2025Water dissociation and rotational broadening in the atmosphere of KELT-20 b from high-resolution spectroscopyFeb 3, 2025Technical description and performance of the phase II version of the Keck Planet Imager and CharacterizerJan 23, 2025HD 206893 B at High Spectral Resolution with the Keck Planet Imager and Characterizer (KPIC)Dec 5, 2024True mass and atmospheric composition of the non-transiting hot Jupiter HD 143105 bNov 22, 2024PDS 70b Shows Stellar-like Carbon-to-oxygen RatioAug 19, 2024RV measurements of directly imaged brown dwarf GQ Lup B to search for exo-satellitesAug 19, 2024Fringing analysis and forward modeling of Keck Planet Imager and Characterizer (KPIC) spectraJul 30, 2024Atmospheric characterization of the super-Jupiter HIP 99770 b with KPICApr 11, 2024Orbital and Atmospheric Characterization of the 1RXS J034231.8+121622 System Using High-Resolution Spectroscopy Confirms That The Companion is a Low-Mass StarMar 26, 2024Vortex Fiber Nulling for Exoplanet Observations: First Direct Detection of M Dwarf Companions around HIP 21543, HIP 94666, and HIP 50319Dec 4, 2023Validation of elemental and isotopic abundances in late-M spectral types with the benchmark HIP 55507 AB systemNov 30, 2023Atmospheric metallicity and C/O of HD 189733 b from high-resolution spectroscopySep 12, 2023Vortex Fiber Nulling for Exoplanet Observations: Implementation and First LightMay 30, 2023Keck/KPIC Emission Spectroscopy of WASP-33bJan 10, 2023Detecting exomoons from radial velocity measurements of self-luminous planets: application to observations of HR 7672 B and future prospectsSep 30, 2022Retrieving C and O Abundance of HR 8799 c by Combining High- and Low-Resolution Data