The California-Kepler survey. III. A gap in the radius distribution of small planets
The size of a planet is an observable property directly connected to the physics of its
formation and evolution. We used precise radius measurements from the California-Kepler …
formation and evolution. We used precise radius measurements from the California-Kepler …
Probabilistic forecasting of the masses and radii of other worlds
Mass and radius are two of the most fundamental properties of an astronomical object.
Increasingly, new planet discoveries are being announced with a measurement of one of …
Increasingly, new planet discoveries are being announced with a measurement of one of …
A compositional link between rocky exoplanets and their host stars
Stars and planets both form by accreting material from a surrounding disk. Because they
grow from the same material, theory predicts that there should be a relationship between …
grow from the same material, theory predicts that there should be a relationship between …
Gaia Data Release 3-Astrometric orbit determination with Markov chain Monte Carlo and genetic algorithms: Systems with stellar, sub-stellar, and planetary mass …
B Holl, A Sozzetti, J Sahlmann, P Giacobbe… - Astronomy & …, 2023 - aanda.org
Context. The astrometric discovery of sub-stellar mass companions orbiting stars is
exceedingly hard due to the required sub-milliarcsecond precision, limiting the application of …
exceedingly hard due to the required sub-milliarcsecond precision, limiting the application of …
Transit detection of the long-period volatile-rich super-Earth ν2 Lupi d with CHEOPS
Exoplanets transiting bright nearby stars are key objects for advancing our knowledge of
planetary formation and evolution. The wealth of photons from the host star gives detailed …
planetary formation and evolution. The wealth of photons from the host star gives detailed …
Compositional imprints in density–distance–time: a rocky composition for close-in low-mass exoplanets from the location of the valley of evaporation
S Jin, C Mordasini - The Astrophysical Journal, 2018 - iopscience.iop.org
We use an end-to-end model of planet formation, thermodynamic evolution, and
atmospheric escape to investigate how the statistical imprints of evaporation depend on the …
atmospheric escape to investigate how the statistical imprints of evaporation depend on the …
A review of planetary systems around HD 99492, HD 147379, and HD 190007 with HARPS-N
Context. The Rocky Planet Search (RPS) program is dedicated to a blind radial velocity (RV)
search of planets around bright stars in the northern hemisphere, using the high-resolution …
search of planets around bright stars in the northern hemisphere, using the high-resolution …
The LCES HIRES/Keck precision radial velocity exoplanet survey
We describe a 20 year survey carried out by the Lick-Carnegie Exoplanet Survey Team
(LCES), using precision radial velocities from HIRES on the Keck I telescope to find and …
(LCES), using precision radial velocities from HIRES on the Keck I telescope to find and …
The 10 parsec sample in the Gaia era
C Reylé, K Jardine, P Fouqué, JA Caballero… - Astronomy & …, 2021 - aanda.org
Context. The nearest stars provide a fundamental constraint for our understanding of stellar
physics and the Galaxy. The nearby sample serves as an anchor where all objects can be …
physics and the Galaxy. The nearby sample serves as an anchor where all objects can be …
Three years of HARPS-N high-resolution spectroscopy and precise radial velocity data for the Sun
X Dumusque, M Cretignier, D Sosnowska… - Astronomy & …, 2021 - aanda.org
Context. The solar telescope connected to HARPS-N has been observing the Sun since the
summer of 2015. Such a high-cadence, long-baseline data set is crucial for understanding …
summer of 2015. Such a high-cadence, long-baseline data set is crucial for understanding …