Showing 1–20 of 27 results
/ Date/ Name
Feb 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 GyrOct 25, 2023The GAPS programme at TNG XLIX. TOI-5398, the youngest compact multi-planet system composed of an inner sub-Neptune and an outer warm SaturnSep 18, 2023TESS Spots a Super-Puff: The Remarkably Low Density of TOI-1420bAug 23, 2022TOI-4562 b: A highly eccentric temperate Jupiter analog orbiting a young field starJan 31, 2022TOI-1268b: the youngest, hot, Saturn-mass transiting exoplanetSep 6, 2021The TESS Mission Target Selection ProcedureMay 18, 2021TIC 172900988: A Transiting Circumbinary Planet Detected in One Sector of TESS DataMar 23, 2021TOI-1634 b: an Ultra-Short Period Keystone Planet Sitting Inside the M Dwarf Radius ValleyMar 23, 2021The TESS Objects of Interest Catalog from the TESS Prime MissionSep 15, 2020A Giant Planet Candidate Transiting a White DwarfSep 9, 2020A super-Earth and a sub-Neptune orbiting the bright, quiet M3 dwarf TOI-1266Mar 30, 2020Retrograde-rotating exoplanets experience obliquity excitations in an eccentricity-enabled resonanceJan 3, 2020The First Habitable Zone Earth-sized Planet from TESS. I: Validation of the TOI-700 SystemJun 2, 2019Two new HATNet hot Jupiters around A stars, and the first glimpse at the occurrence rate of hot Jupiters from TESSMar 19, 2019The L 98-59 System: Three Transiting, Terrestrial-Sized Planets Orbiting a Nearby M-dwarfOct 18, 2017Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25Dec 1, 2015Kepler-1647b: the largest and longest-period Kepler transiting circumbinary planetFeb 6, 2015Planetary Candidates Observed by Kepler VI: Planet Sample from Q1-Q16 (47 Months)Feb 26, 2014Validation of Kepler's Multiple Planet Candidates. III: Light Curve Analysis & Announcement of Hundreds of New Multi-planet SystemsFeb 15, 2013Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65