Showing 1–20 of 43 results
/ Date/ Name
Sep 18, 2025Detection and characterisation of a 106-day transiting Jupiter : TOI-2449 b / NGTS-36 bJul 30, 2024TOI-757 b: an eccentric transiting mini-Neptune on a 17.5-d orbitJun 23, 2024Discovery of a cold giant planet and mass measurement of a hot super-Earth in the multi-planetary system WASP-132Jun 3, 2024CHEOPS in-flight performance: A comprehensive look at the first 3.5 years of operationsMar 25, 2024Precise characterisation of HD 15337 with CHEOPS: a laboratory for planet formation and evolutionNov 29, 2023A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067Oct 20, 2023A hot mini-Neptune and a temperate, highly eccentric sub-Saturn around the bright K-dwarf TOI-2134Jun 7, 2023TOI-5678 b: A 48-day transiting Neptune-mass planet characterized with CHEOPS and HARPSMar 29, 2023Near-IR and optical radial velocities of the active M dwarf star Gl 388 (AD Leo) with SPIRou at CFHT and SOPHIE at OHP: A 2.23 day rotation period and no evidence for a corotating planetFeb 21, 2023TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPSJul 28, 2022The HD 93963 A transiting system: A 1.04d super-Earth and a 3.65 d sub-Neptune discovered by TESS and CHEOPSJan 19, 2022Investigating the architecture and internal structure of the TOI-561 system planets with CHEOPS, HARPS-N and TESSOct 25, 2021The young HD 73583 (TOI-560) planetary system: Two 10-M$_\oplus$ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarfMay 5, 2021TESS and HARPS reveal two sub-Neptunes around TOI 1062Apr 30, 2021TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrAMar 25, 2021New binaries from the SHINE surveyMar 23, 2021TOI-1634 b: an Ultra-Short Period Keystone Planet Sitting Inside the M Dwarf Radius ValleyJan 12, 2021A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113Jan 5, 2021Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valleyOct 30, 2020Separating planetary reflex Doppler shifts from stellar variability in the wavelength domain