Showing 1–20 of 38 results
/ Date/ Name
Aug 22, 2025The HD 60779 Planetary System: A Transiting Sub-Neptune on a 30-day Orbit and a More Massive Outer WorldJun 25, 2025The mass of the exo-Venus Gliese 12 b, as revealed by HARPS-N, ESPRESSO, and CARMENESOct 23, 2024Further study of starspot activity and measurement of differential rotation for SZ PisciumJul 30, 2024TOI-757 b: an eccentric transiting mini-Neptune on a 17.5-d orbitJun 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 HARPSFeb 21, 2023TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPSFeb 1, 2023Magnetic topologies of two weak-line T Tauri stars TAP 4 and TAP 40Aug 25, 2022Validation of TESS exoplanet candidates orbiting solar analogues in the all-sky PLATO input catalogueJul 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 TESSMay 19, 2021Estimating Magnetic Filling Factors From Simultaneous Spectroscopy and Photometry: Disentangling Spots, Plage, and NetworkMar 23, 2021TOI-1634 b: an Ultra-Short Period Keystone Planet Sitting Inside the M Dwarf Radius ValleyOct 30, 2020Separating planetary reflex Doppler shifts from stellar variability in the wavelength domainOct 30, 2020Identifying Exoplanets with Deep Learning. IV. Removing Stellar Activity Signals from Radial Velocity Measurements Using Neural NetworksMay 6, 2020Doppler imaging and differential rotation of $σ^{2}$ Coronae Borealis using SONGJan 8, 2020The first Doppler imaging of the active binary prototype RS Canum Venaticorum