State of the field: extreme precision radial velocities
DA Fischer, G Anglada-Escude… - Publications of the …, 2016 - iopscience.iop.org
Abstract The Second Workshop on Extreme Precision Radial Velocities defined circa 2015
the state of the art Doppler precision and identified the critical path challenges for reaching …
the state of the art Doppler precision and identified the critical path challenges for reaching …
The California Legacy Survey. I. A catalog of 178 planets from precision radial velocity monitoring of 719 nearby stars over three decades
LJ Rosenthal, BJ Fulton, LA Hirsch… - The Astrophysical …, 2021 - iopscience.iop.org
We present a high-precision radial velocity (RV) survey of 719 FGKM stars, which host 164
known exoplanets and 14 newly discovered or revised exoplanets and substellar …
known exoplanets and 14 newly discovered or revised exoplanets and substellar …
Prevalence of Earth-size planets orbiting Sun-like stars
EA Petigura, AW Howard… - Proceedings of the …, 2013 - National Acad Sciences
Determining whether Earth-like planets are common or rare looms as a touchstone in the
question of life in the universe. We searched for Earth-size planets that cross in front of their …
question of life in the universe. We searched for Earth-size planets that cross in front of their …
Giant planet occurrence in the stellar mass-metallicity plane
Correlations between stellar properties and the occurrence rate of exoplanets can be used
to inform the target selection of future planet-search efforts and provide valuable clues about …
to inform the target selection of future planet-search efforts and provide valuable clues about …
Spectroscopic properties of cool stars (SPOCS). I. 1040 F, G, and K dwarfs from Keck, Lick, and AAT planet search programs
JA Valenti, DA Fischer - The Astrophysical Journal Supplement …, 2005 - iopscience.iop.org
We present a uniform catalog of stellar properties for 1040 nearby F, G, and K stars that have
been observed by the Keck, Lick, and AAT planet search programs. Fitting observed echelle …
been observed by the Keck, Lick, and AAT planet search programs. Fitting observed echelle …
The frequency of hot Jupiters orbiting nearby solar-type stars
We determine the fraction of F, G, and K dwarfs in the solar neighborhood hosting hot
Jupiters as measured by the California Planet Survey from the Lick and Keck planet …
Jupiters as measured by the California Planet Survey from the Lick and Keck planet …
Catalog of nearby exoplanets
We present a catalog of nearby exoplanets. It contains the 172 known low-mass
companions with orbits established through radial velocity and transit measurements around …
companions with orbits established through radial velocity and transit measurements around …
Origins of eccentric extrasolar planets: testing the planet-planet scattering model
In planetary systems with two or more giant planets, dynamical instabilities can lead to
collisions or ejections through strong planet-planet scattering. Previous studies for initial …
collisions or ejections through strong planet-planet scattering. Previous studies for initial …
A new planet around an M dwarf: revealing a correlation between exoplanets and stellar mass
JA Johnson, RP Butler, GW Marcy… - The Astrophysical …, 2007 - iopscience.iop.org
We report precise Doppler measurements of GJ 317 (M3. 5 V) that reveal the presence of a
planet with a minimum mass MP sin i= 1.2 M Jup in an eccentric, 692.9 day orbit. GJ 317 is …
planet with a minimum mass MP sin i= 1.2 M Jup in an eccentric, 692.9 day orbit. GJ 317 is …
Prospects for the characterization and confirmation of transiting exoplanets via the Rossiter-McLaughlin effect
BS Gaudi, JN Winn - The Astrophysical Journal, 2007 - iopscience.iop.org
Abstract The Rossiter-McLaughlin (RM) effect is the distortion of stellar spectral lines that
occurs during eclipses or transits, due to stellar rotation. We assess the future prospects for …
occurs during eclipses or transits, due to stellar rotation. We assess the future prospects for …