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 …
Hidden water in magma ocean exoplanets
C Dorn, T Lichtenberg - The Astrophysical Journal Letters, 2021 - iopscience.iop.org
We demonstrate that the deep volatile storage capacity of magma oceans has significant
implications for the bulk composition, interior, and climate state inferred from exoplanet mass …
implications for the bulk composition, interior, and climate state inferred from exoplanet mass …
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 …
K2 and Spitzer phase curves of the rocky ultra-short-period planet K2-141 b hint at a tenuous rock vapor atmosphere
K2-141 b is a transiting, small (1.5 R⊕) ultra-short-period (USP) planet discovered by the
Kepler space telescope orbiting a K-dwarf host star every 6.7 h. The planet's high surface …
Kepler space telescope orbiting a K-dwarf host star every 6.7 h. The planet's high surface …
On the application of Bayesian leave-one-out cross-validation to exoplanet atmospheric analysis
Over the last decade exoplanetary transmission spectra have yielded an unprecedented
understanding about the physical and chemical nature of planets outside our solar system …
understanding about the physical and chemical nature of planets outside our solar system …
Investigating the architecture and internal structure of the TOI-561 system planets with CHEOPS, HARPS-N, and TESS
G Lacedelli, TG Wilson, L Malavolta… - Monthly Notices of …, 2022 - academic.oup.com
We present a precise characterization of the TOI-561 planetary system obtained by
combining previously published data with TESS and CHEOPS photometry, and a new set of …
combining previously published data with TESS and CHEOPS photometry, and a new set of …
Exfoliated 2D Layered and Nonlayered Metal Phosphorous Trichalcogenides Nanosheets as Promising Electrocatalysts for CO2 Reduction
Abstract Two‐dimensional (2D) materials catalysts provide an atomic‐scale view on a
fascinating arena for understanding the mechanism of electrocatalytic carbon dioxide …
fascinating arena for understanding the mechanism of electrocatalytic carbon dioxide …
Investigating the visible phase-curve variability of 55 Cnc e
Context. 55 Cnc e is an ultra-short period super-Earth transiting a Sun-like star. Previous
observations in the optical range detected a time-variable flux modulation that is phased …
observations in the optical range detected a time-variable flux modulation that is phased …
Spi-OPS: Spitzer and CHEOPS confirm the near-polar orbit of MASCARA-1 b and reveal a hint of dayside reflection
Context. The light curves of tidally locked hot Jupiters transiting fast-rotating, early-type stars
are a rich source of information about both the planet and star, with full-phase coverage …
are a rich source of information about both the planet and star, with full-phase coverage …