HARPS XXXI. The M-dwarf sample Virtual Observatory Resource

Authors

1. Bonfils X.
2. Delfosse X.
3. Udry S.
4. Forveille T.
5. Mayor M.
6. Perrier C.,Bouchy F.
7. Gillon M.
8. Lovis C.
9. Pepe F.
10. Queloz D.
11. Santos N.C.,Segransan D.
12. Bertaux J.-L.

Published by

CDS

Abstract

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

Keywords

1. multiple-stars
2. solar-system-planets
3. dwarf-stars
4. m-stars

Bibliographic source Bibcode

2013A&A...549A.109B

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/549/A109

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/549/A109

Document Object Identifer DOI

doi:10.26093/cds/vizier.35490109

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/549/A109
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/549/A109
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/549/A109

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Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/549/A109/table3?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/549/A109/table3?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/549/A109/table3?