Extreme solar events
EW Cliver, CJ Schrijver, K Shibata… - Living Reviews in Solar …, 2022 - Springer
We trace the evolution of research on extreme solar and solar-terrestrial events from the
1859 Carrington event to the rapid development of the last twenty years. Our focus is on the …
1859 Carrington event to the rapid development of the last twenty years. Our focus is on the …
Atmospheres of rocky exoplanets
R Wordsworth, L Kreidberg - Annual Review of Astronomy and …, 2022 - annualreviews.org
Rocky planets are common around other stars, but their atmospheric properties remain
largely unconstrained. Thanks to a wealth of recent planet discoveries and upcoming …
largely unconstrained. Thanks to a wealth of recent planet discoveries and upcoming …
ESPRESSO at VLT-On-sky performance and first results
Context. ESPRESSO is the new high-resolution spectrograph of ESO's Very Large
Telescope (VLT). It was designed for ultra-high radial-velocity (RV) precision and extreme …
Telescope (VLT). It was designed for ultra-high radial-velocity (RV) precision and extreme …
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 …
The evaporation valley in the Kepler planets
A new piece of evidence supporting the photoevaporation-driven evolution model for low-
mass, close-in exoplanets was recently presented by the California–Kepler Survey. The …
mass, close-in exoplanets was recently presented by the California–Kepler Survey. The …
Identifying exoplanets with deep learning: A five-planet resonant chain around kepler-80 and an eighth planet around kepler-90
Abstract NASA's Kepler Space Telescope was designed to determine the frequency of Earth-
sized planets orbiting Sun-like stars, but these planets are on the very edge of the mission's …
sized planets orbiting Sun-like stars, but these planets are on the very edge of the mission's …
Disks around t tauri stars with sphere (dartts-s). i. sphere/irdis polarimetric imaging of eight prominent t tauri disks
We present the first part of our Disks ARound T Tauri Stars with SPHERE (DARTTS-S)
survey: observations of eight T Tauri stars that were selected based on their strong (sub) …
survey: observations of eight T Tauri stars that were selected based on their strong (sub) …
The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity
CD Dressing, D Charbonneau - The Astrophysical Journal, 2015 - iopscience.iop.org
We present an improved estimate of the occurrence rate of small planets orbiting small stars
by searching the full four-year Kepler data set for transiting planets using our own planet …
by searching the full four-year Kepler data set for transiting planets using our own planet …
Kepler data validation I—architecture, diagnostic tests, and data products for vetting transiting planet candidates
Abstract The Kepler Mission was designed to identify and characterize transiting planets in
the Kepler Field of View and to determine their occurrence rates. Emphasis was placed on …
the Kepler Field of View and to determine their occurrence rates. Emphasis was placed on …
Most 1.6 Earth-radius planets are not rocky
LA Rogers - The Astrophysical Journal, 2015 - iopscience.iop.org
The Kepler mission, combined with ground-based radial velocity (RV) follow-up and
dynamical analyses of transit timing variations, has revolutionized the observational …
dynamical analyses of transit timing variations, has revolutionized the observational …