The occurrence and architecture of exoplanetary systems
JN Winn, DC Fabrycky - Annual Review of Astronomy and …, 2015 - annualreviews.org
The basic geometry of the Solar System—the shapes, spacings, and orientations of the
planetary orbits—has long been a subject of fascination as well as inspiration for planet …
planetary orbits—has long been a subject of fascination as well as inspiration for planet …
[HTML][HTML] The CARMENES search for exoplanets around M dwarfs-First visual-channel radial-velocity measurements and orbital parameter updates of seven M-dwarf …
T Trifonov, M Kürster, M Zechmeister, L Tal-Or… - Astronomy & …, 2018 - aanda.org
Context. The main goal of the CARMENES survey is to find Earth-mass planets around
nearby M-dwarf stars. Seven M dwarfs included in the CARMENES sample had been …
nearby M-dwarf stars. Seven M dwarfs included in the CARMENES sample had been …
WARM JUPITERS FROM SECULAR PLANET–PLANET INTERACTIONS
C Petrovich, S Tremaine - The Astrophysical Journal, 2016 - iopscience.iop.org
Most warm Jupiters (gas-giant planets with $0.1\,{\rm {au}}\lesssim a\lesssim 1$ au) have
pericenter distances that are too large for significant orbital migration by tidal friction. We …
pericenter distances that are too large for significant orbital migration by tidal friction. We …
TTVFast: an efficient and accurate code for transit timing inversion problems
KM Deck, E Agol, MJ Holman… - The Astrophysical …, 2014 - iopscience.iop.org
Transit timing variations (TTVs) have proven to be a powerful technique for confirming
Kepler planet candidates, for detecting non-transiting planets, and for constraining the …
Kepler planet candidates, for detecting non-transiting planets, and for constraining the …
TOI-2525 b and c: A Pair of Massive Warm Giant Planets with Strong Transit Timing Variations Revealed by TESS
TOI-2525 b and c: A Pair of Massive Warm Giant Planets with Strong Transit Timing Variations
Revealed by TESS - IOPscience Skip to content IOP Science home Accessibility Help Search …
Revealed by TESS - IOPscience Skip to content IOP Science home Accessibility Help Search …
Astrophysical Insights into Radial Velocity Jitter from an Analysis of 600 Planet-search Stars
Radial velocity (RV) detection of planets is hampered by astrophysical processes on the
surfaces of stars that induce a stochastic signal, or" jitter," which can drown out or even …
surfaces of stars that induce a stochastic signal, or" jitter," which can drown out or even …
Limits on planetary companions from Doppler surveys of nearby stars
Most of our knowledge of planets orbiting nearby stars comes from Doppler surveys. For
spaced-based, high-contrast imaging missions, nearby stars with Doppler-discovered …
spaced-based, high-contrast imaging missions, nearby stars with Doppler-discovered …
Dynamical evolution induced by Planet Nine
K Batygin, A Morbidelli - The Astronomical Journal, 2017 - iopscience.iop.org
Dynamical Evolution Induced by Planet Nine - IOPscience This site uses cookies. By continuing
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A pair of warm giant planets near the 2: 1 mean motion resonance around the K-dwarf star TOI-2202
TOI-2202 b is a transiting warm Jovian-mass planet with an orbital period of P= 11.91 days
identified from the Full Frame Images data of five different sectors of the TESS mission. Ten …
identified from the Full Frame Images data of five different sectors of the TESS mission. Ten …
A general stability-driven approach for the refinement of multi-planet systems
M Stalport, JB Delisle, S Udry, EC Matthews… - Astronomy & …, 2022 - aanda.org
Context. Over recent years, the number of detected multi-planet systems has grown
significantly. An important subclass of these are the compact configurations. Precise …
significantly. An important subclass of these are the compact configurations. Precise …