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ESO/HARPS Radial Velocities Catalog

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arxiv 2312.06586 v2 pith:WFPXRSV5 submitted 2023-12-11 astro-ph.SR astro-ph.EPastro-ph.IM

classification astro-ph.SRastro-ph.EPastro-ph.IM
keywords radialvelocitiescatalogharpsastronomicalobjectobtainedalpha
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

This document details the first public data release of the HARPS radial velocities catalog. This data release aims to provide the astronomical community with a catalog of radial velocities obtained with spectroscopic observations acquired from 2003 to 2023 with the High Accuracy Radial Velocity Planet Searcher (HARPS) spectrograph installed at the ESO 3.6m telescope in La Silla Observatory (Chile), and spanning wavelengths from 3800 to 6900 Angstrom. The catalog comprises 289843 observations of 6488 unique astronomical objects. Radial velocities reported in this catalog are obtained using the HARPS pipeline, with a typical precision of 0.5 m/s, which is essential for the search and validation of exoplanets. Additionally, independent radial velocities measured on the H$\alpha$ spectral line are included, with a typical error of around 300 m/s suitable for various astrophysical applications where high precision is not critical. This catalog includes 282294 radial velocities obtained through the HARPS pipeline and 288972 derived from the H$_\alpha$ line, collectively forming a time-series dataset that provides a historical record of measurements for each object. Further, each object has been cross-referenced with the SIMBAD astronomical database to ensure accurate identification, enabling users to locate and verify objects with existing records in astronomical literature. Information provided for each object includes: astrometric parameters (coordinates, parallaxes, proper motions, radial velocities), photometric parameters (apparent magnitudes in the visible and near-infrared), spectral types and object classifications.

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  1. Constraining nearby substellar companion architectures using High Contrast Imaging, Radial Velocity and Astrometry data

    astro-ph.EP 2025-07 conditional novelty 5.0 of 10

    For seven nearby M dwarfs, combining imaging, radial velocity, and astrometry raises the fraction of detectable substellar companions beyond any single method, though no new companions were found.

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