Measuring precise radial velocities on individual spectral lines - I. Validation of the method and application to mitigate stellar activity,
A&A, 620 (2018) A47
Published online: 2018-11-29
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APERO: A PipelinE to Reduce Observations—Demonstration with SPIRou
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An Interpretable Machine-learning Framework for Modeling High-resolution Spectroscopic Data*
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Leveraging Space-based Data from the Nearest Solar-type Star to Better Understand Stellar Activity Signatures in Radial Velocity Data
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TESS Asteroseismology of α Mensae: Benchmark Ages for a G7 Dwarf and Its M Dwarf Companion
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Precision Millimeter Astrometry of the α Centauri AB System
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Three years of HARPS-N high-resolution spectroscopy and precise radial velocity data for the Sun
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EXPRES. II. Searching for Planets around Active Stars: A Case Study of HD 101501
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Friends and Foes: Conditional Occurrence Rates of Exoplanet Companions and Their Impact on Radial Velocity Follow-up Surveys
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A HARPS-N mass for the elusive Kepler-37d: a case study in disentangling stellar activity and planetary signals
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The Rossiter–McLaughlin effect revolutions: an ultra-short period planet and a warm mini-Neptune on perpendicular orbits
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