A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067
Planets with radii between that of the Earth and Neptune (hereafter referred to as 'sub-
Neptunes') are found in close-in orbits around more than half of all Sun-like stars,. However …
Neptunes') are found in close-in orbits around more than half of all Sun-like stars,. However …
A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS
We report the discovery and characterization of a pair of sub-Neptunes transiting the bright K-
dwarf TOI-1064 (TIC 79748331), initially detected in the Transiting Exoplanet Survey …
dwarf TOI-1064 (TIC 79748331), initially detected in the Transiting Exoplanet Survey …
Analysis of Early Science observations with the CHaracterising ExOPlanets Satellite (CHEOPS) using pycheops
PFL Maxted, D Ehrenreich, TG Wilson… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT CHEOPS (CHaracterising ExOPlanet Satellite) is an ESA S-class mission that
observes bright stars at high cadence from low-Earth orbit. The main aim of the mission is to …
observes bright stars at high cadence from low-Earth orbit. The main aim of the mission is to …
Detection of the tidal deformation of WASP-103b at 3 σ with CHEOPS
Context. Ultra-short period planets undergo strong tidal interactions with their host star which
lead to planet deformation and orbital tidal decay. Aims. WASP-103b is the exoplanet with …
lead to planet deformation and orbital tidal decay. Aims. WASP-103b is the exoplanet with …
The atmosphere and architecture of WASP-189 b probed by its CHEOPS phase curve
A Deline, MJ Hooton, M Lendl, B Morris… - Astronomy & …, 2022 - aanda.org
Context. Gas giants orbiting close to hot and massive early-type stars can reach dayside
temperatures that are comparable to those of the coldest stars. These 'ultra-hot Jupiters' …
temperatures that are comparable to those of the coldest stars. These 'ultra-hot Jupiters' …
The changing face of AU Mic b: stellar spots, spin-orbit commensurability, and transit timing variations as seen by CHEOPS and TESS
GM Szabó, D Gandolfi, A Brandeker… - Astronomy & …, 2021 - aanda.org
AU Mic is a young planetary system with a resolved debris disc showing signs of planet
formation and two transiting warm Neptunes near mean-motion resonances. Here we …
formation and two transiting warm Neptunes near mean-motion resonances. Here we …
TOI-5678b: A 48-day transiting Neptune-mass planet characterized with CHEOPS and HARPS
Context. A large sample of long-period giant planets has been discovered thanks to long-
term radial velocity surveys, but only a few dozen of these planets have a precise radius …
term radial velocity surveys, but only a few dozen of these planets have a precise radius …
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d
Context. Multi-planet systems are important sources of information regarding the evolution of
planets. However, the long-period planets in these systems often escape detection. These …
planets. However, the long-period planets in these systems often escape detection. These …
The Ariel Target List: The Impact of TESS and the Potential for Characterizing Multiple Planets within a System
B Edwards, G Tinetti - The Astronomical Journal, 2022 - iopscience.iop.org
The Ariel Target List: The Impact of TESS and the Potential for Characterizing Multiple Planets
within a System - IOPscience This site uses cookies. By continuing to use this site you agree to …
within a System - IOPscience This site uses cookies. By continuing to use this site you agree to …
TESS and CHEOPS discover two warm sub-Neptunes transiting the bright K-dwarf HD 15906
We report the discovery of two warm sub-Neptunes transiting the bright (G= 9.5 mag) K-
dwarf HD 15906 (TOI 461, TIC 4646810). This star was observed by the Transiting …
dwarf HD 15906 (TOI 461, TIC 4646810). This star was observed by the Transiting …