Stellar obliquities in exoplanetary systems
SH Albrecht, RI Dawson, JN Winn - Publications of the …, 2022 - iopscience.iop.org
The rotation of a star and the revolutions of its planets are not necessarily aligned. This
article reviews the measurement techniques, key findings, and theoretical interpretations …
article reviews the measurement techniques, key findings, and theoretical interpretations …
Overview of the LAMOST survey in the first decade
The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), also known as
the Guoshoujing Telescope, is a major national scientific facility for astronomical research …
the Guoshoujing Telescope, is a major national scientific facility for astronomical research …
A revised exoplanet yield from the transiting exoplanet survey satellite (TESS)
Abstract The Transiting Exoplanet Survey Satellite (TESS) has a goal of detecting small
planets orbiting stars bright enough for mass determination via ground-based radial velocity …
planets orbiting stars bright enough for mass determination via ground-based radial velocity …
SOAR TESS survey. I. Sculpting of TESS planetary systems by stellar companions
Abstract The Transiting Exoplanet Survey Satellite (TESS) is finding transiting planet
candidates around bright, nearby stars across the entire sky. The large field of view …
candidates around bright, nearby stars across the entire sky. The large field of view …
The California-Kepler survey. V. Peas in a pod: Planets in a Kepler multi-planet system are similar in size and regularly spaced
We have established precise planet radii, semimajor axes, incident stellar fluxes, and stellar
masses for 909 planets in 355 multi-planet systems discovered by Kepler. In this sample, we …
masses for 909 planets in 355 multi-planet systems discovered by Kepler. In this sample, we …
The Gaia–Kepler Stellar Properties Catalog. II. Planet radius demographics as a function of stellar mass and age
TA Berger, D Huber, E Gaidos… - The Astronomical …, 2020 - iopscience.iop.org
Studies of exoplanet demographics require large samples and precise constraints on
exoplanet host stars. Using the homogeneous Kepler stellar properties derived using the …
exoplanet host stars. Using the homogeneous Kepler stellar properties derived using the …
Breaking the chains: hot super-Earth systems from migration and disruption of compact resonant chains
Abstract 'Hot super-Earths'(or 'mini-Neptunes') between one and four times Earth's size with
period shorter than 100 d orbit 30–50 per cent of Sun-like stars. Their orbital configuration …
period shorter than 100 d orbit 30–50 per cent of Sun-like stars. Their orbital configuration …
The orbital eccentricity of small planet systems
V Van Eylen, S Albrecht, X Huang… - The Astronomical …, 2019 - iopscience.iop.org
We determine the orbital eccentricities of individual small Kepler planets, through a
combination of asteroseismology and transit light-curve analysis. We are able to constrain …
combination of asteroseismology and transit light-curve analysis. We are able to constrain …
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 …
The New Generation Planetary Population Synthesis (NGPPS)-I. Bern global model of planet formation and evolution, model tests, and emerging planetary systems
Context. The explosion of observational data on exoplanets gives many constraints on
theoretical models of planet formation and evolution. Observational data probe very large …
theoretical models of planet formation and evolution. Observational data probe very large …