Disentangling between stellar activity and planetary signals
A&A, 528 (2011) A4
Published online: 2011-02-16
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The CARMENES search for exoplanets around M dwarfs
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The SOPHIE search for northern extrasolar planets
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Four Jovian planets around low-luminosity giant stars observed by the EXPRESS and PPPS
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A Stellar Activity F-statistic for Exoplanet Surveys (SAFE)
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The Habitable-zone Planet Finder Detects a Terrestrial-mass Planet Candidate Closely Orbiting Gliese 1151: The Likely Source of Coherent Low-frequency Radio Emission from an Inactive Star
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A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113
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EXPRES. II. Searching for Planets around Active Stars: A Case Study of HD 101501
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YARARA: Significant improvement in RV precision through post-processing of spectral time series
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A remnant planetary core in the hot-Neptune desert
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Decoding the radial velocity variations of HD 41248 with ESPRESSO
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The CARMENES search for exoplanets around M dwarfs
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FIESTA – disentangling stellar variability from exoplanets in the Fourier domain
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The correlation between photometric variability and radial velocity jitter
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Transiting exoplanets from the CoRoT space mission
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Photometry as a Proxy for Stellar Activity in Radial Velocity Analyses
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The CARMENES search for exoplanets around M dwarfs
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HD 199719’un Çizgi Ortay Analizi
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Measuring precise radial velocities on individual spectral lines
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The Magellan/PFS Exoplanet Search: a 55-d period dense Neptune transiting the bright (V = 8.6) star HD 95338
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A robust, template-free approach to precise radial velocity extraction
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Persistent Starspot Signals on M Dwarfs: Multiwavelength Doppler Observations with the Habitable-zone Planet Finder and Keck/HIRES
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USuRPER: Unit-sphere representation periodogram for full spectra
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The HARPS search for southern extra-solar planets
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Detection and characterisation of 54 massive companions with the SOPHIE spectrograph
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Filtering Solar-Like Oscillations for Exoplanet Detection in Radial Velocity Observations
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The Impact of Stellar Surface Magnetoconvection and Oscillations on the Detection of Temperate, Earth-Mass Planets Around Sun-Like Stars
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Reducing activity-induced variations in a radial-velocity time series of the Sun as a star
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The imprint of X-ray photoevaporation of planet-forming discs on the orbital distribution of giant planets
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So close, so different: characterization of the K2-36 planetary system with HARPS-N
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Hot, rocky and warm, puffy super-Earths orbiting TOI-402 (HD 15337)
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Multi-wavelength variability of the young solar analog ι Horologii
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Stellar Surface Magnetoconvection as a Source of Astrophysical Noise. III. Sun-as-a-Star Simulations and Optimal Noise Diagnostics
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