Results 11 to 20 of about 2,565,021 (373)

Photometry as a proxy for stellar activity in radial velocity analyses [PDF]

open access: yesAstronomical Journal, 2020
Stellar activity remains a limiting factor in measuring precise planet parameters from radial velocity spectroscopy, not least in the search for Earth mass planets orbiting in the habitable zones of Sun-like stars.
Crossfield, Ian J. M.   +1 more
core   +2 more sources

RadVel: The Radial Velocity Modeling Toolkit [PDF]

open access: yes, 2018
RadVel is an open source Python package for modeling Keplerian orbits in radial velocity (RV) time series. RadVel provides a convenient framework to fit RVs using maximum a posteriori optimization and to compute robust confidence intervals by sampling ...
Blunt, Sarah   +3 more
core   +4 more sources

The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades [PDF]

open access: yesAstrophysical Journal Supplement Series, 2021
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 companions.
L. Rosenthal   +22 more
semanticscholar   +1 more source

orvara: An Efficient Code to Fit Orbits Using Radial Velocity, Absolute, and/or Relative Astrometry [PDF]

open access: yesAstronomical Journal, 2021
We present an open-source Python package, Orbits from Radial Velocity, Absolute, and/or Relative Astrometry (orvara), to fit Keplerian orbits to any combination of radial velocity, relative astrometry, and absolute astrometry data from the Hipparcos-Gaia
Timothy D. Brandt   +7 more
semanticscholar   +1 more source

The Solar Neighborhood XLVIII: Nine Giant Planets Orbiting Nearby K Dwarfs, and the CHIRON Spectrograph’s Radial Velocity Performance [PDF]

open access: yesAstronomical Journal, 2021
We report initial results of a large radial velocity survey of K dwarfs up to a distance of 50 pc from the solar system, to look for stellar, brown dwarf, and Jovian planets using radial velocities from the CHIRON spectrograph on the CTIO/SMARTS 1.5 m ...
L. Paredes   +7 more
semanticscholar   +1 more source

Public HARPS radial velocity database corrected for systematic errors [PDF]

open access: yesAstronomy & Astrophysics, 2020
Context. The High Accuracy Radial velocity Planet Searcher (HARPS) spectrograph has been mounted since 2003 at the ESO 3.6 m telescope in La Silla and provides state-of-the-art stellar radial velocity (RV) measurements with a precision down to ∼1 m s−1 ...
T. Trifonov   +5 more
semanticscholar   +1 more source

The Sixth Data Release of the Radial Velocity Experiment (RAVE). I. Survey Description, Spectra, and Radial Velocities [PDF]

open access: yesAstronomical Journal, 2020
The Radial Velocity Experiment (Rave) is a magnitude-limited (9 < I < 12) spectroscopic survey of Galactic stars randomly selected in Earth’s southern hemisphere.
M. Steinmetz   +61 more
semanticscholar   +1 more source

Direct confirmation of the radial-velocity planetβPictoris c [PDF]

open access: yesAstronomy & Astrophysics, 2020
Context.Methods used to detect giant exoplanets can be broadly divided into two categories: indirect and direct. Indirect methods are more sensitive to planets with a small orbital period, whereas direct detection is more sensitive to planets orbiting at
M. Nowak   +93 more
semanticscholar   +1 more source

On-sky commissioning of MAROON-X: a new precision radial velocity spectrograph for Gemini North [PDF]

open access: yesGround-based and Airborne Instrumentation for Astronomy VIII, 2020
MAROON-X is a fiber-fed, red-optical, high precision radial velocity spectrograph recently commissioned at the Gemini North telescope on Mauna Kea, Hawai’i.
A. Seifahrt   +12 more
semanticscholar   +1 more source

Three years of HARPS-N high-resolution spectroscopy and precise radial velocity data for the Sun [PDF]

open access: yesAstronomy & Astrophysics, 2020
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 spurious radial-velocity signals induced by our Sun and by the instrument.
X. Dumusque   +37 more
semanticscholar   +1 more source

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