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Table · dataset · 2013

HARPS XXXI. The M-dwarf sample

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Searching for planets around stars with different masses helps us to assess the outcome of planetary formation for different initial conditions.

Description

The low-mass M dwarfs are also the most frequent stars in our Galaxy and potentially therefore, the most frequent planet hosts. We present observations of 102 southern nearby M dwarfs, using a fraction of our guaranteed time on the ESO/HARPS spectrograph.

We observed for 460 h and gathered 1965 precise (~1-3m/s) radial velocities (RVs), spanning the period from Feb. 11, 2003 to Apr. 1, 2009.

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Astronomical sciences 71%
Provenance · 1 source records, 8 field assertions
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concepts[field].anzsrc:group:5101enrichment · IVOA Registrytaxonomy-embedding@1.1.0title+keywords+description (71%)
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