Showing 1–20 of 30 results
/ Date/ Name
Feb 2, 2026Unraveling the Brown Dwarf Desert: Four New Discoveries and a Unifying, Period-Coded PictureSep 18, 2025Detection and characterisation of a 106-day transiting Jupiter : TOI-2449 b / NGTS-36 bApr 7, 2025Investigating the eccentricity distribution of transiting, long-period giant planetsJul 30, 2024TOI-757 b: an eccentric transiting mini-Neptune on a 17.5-d orbitJun 25, 2024Revising Properties of Planet-Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems is Dependent on Stellar SeparationNov 20, 2023The GAPS Programme at TNG L -- TOI-4515 b: An eccentric warm Jupiter orbiting a 1.2 Gyr-old G-starOct 20, 2023A hot mini-Neptune and a temperate, highly eccentric sub-Saturn around the bright K-dwarf TOI-2134Mar 27, 2023The GAPS Programme at TNG XLII. A characterisation study of the multi-planet system around the 400 Myr-old star HD 63433 (TOI-1726)Mar 27, 2023Three Saturn-mass planets transiting F-type stars revealed with TESS and HARPSFeb 16, 2023Revising Properties of Planet-Host Binary Systems. III. There is No Observed Radius Gap For Kepler Planets in Binary Star SystemsNov 4, 2022HD 20329b: An ultra-short-period planet around a solar-type star found by TESSAug 23, 2022TOI-4562 b: A highly eccentric temperate Jupiter analog orbiting a young field starJul 28, 2022GJ 3090 b: one of the most favourable mini-Neptune for atmospheric characterisationJun 24, 2022Revising Properties of Planet-host Binary Systems I.: Methods and Pilot StudyJul 1, 2021Low-Cost Access to the Deep, High-Cadence Sky: the Argus Optical ArrayApr 30, 2021TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrAJan 12, 2021A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113Sep 15, 2020A Giant Planet Candidate Transiting a White DwarfSep 7, 2020The TESS-Keck Survey II: An Ultra-Short Period Rocky Planet and its Siblings Transiting the Galactic Thick-Disk Star TOI-561Jun 12, 2020Constraints on the Physical Properties of GW190814 through Simulations based on DECam Follow-up Observations by the Dark Energy Survey