WASP-31b photometry and radial velocities Virtual Observatory Resource

Authors

1. Anderson D.R.
2. Collier Cameron A.
3. Hellier C.
4. Lendl M.
5. Lister T.A.,Maxted P.F.L.
6. Queloz D.
7. Smalley B.
8. Smith A.M.S.
9. Triaud A.H.M.J.,West R.G.
10. Brown D.J.A.
11. Gillon M.
12. Pepe F.
13. Pollacco D.
14. Segransan D.,Street R.A.
15. Udry S.

Published by

CDS

Abstract

We report the discovery of the low-density, transiting giant planet WASP-31b. The planet is 0.48 Jupiter masses and 1.55 Jupiter radii. It is in a 3.4-day orbit around a metal-poor, late-F-type, V=11.7 dwarf star, which is a member of a common proper motion pair. In terms of its low density, WASP-31b is second only to WASP-17b, which is a more highly irradiated planet of similar mass.

Keywords

1. eclipsing-binary-stars
2. solar-system-planets
3. radial-velocity
4. photometry

Bibliographic source Bibcode

2011A&A...531A..60A

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/531/A60

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/531/A60

Document Object Identifer DOI

doi:10.26093/cds/vizier.35310060

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/531/A60
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/531/A60
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/531/A60

IVOA Table Access TAP

https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).