Limits on Surface Gravities of Kepler Planet-candidate Host Stars from Non-detection of Solar-like Oscillations

Research output: Contribution to journal/Conference contribution in journal/Contribution to newspaperJournal article

    T. L. Campante, School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK campante@bison.ph.bham.ac.uk, W. J. Chaplin, School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK,
  • M. N. Lund
  • D. Huber, NASA Ames Research Center, MS 244-30, Moffett Field, CA 94035, USA, S. Hekker, Astronomical Institute, "Anton Pannekoek," University of Amsterdam, Amsterdam, The Netherlands, R. A. García, Laboratoire AIM, CEA/DSM-CNRS-Université Paris Diderot, E. Corsaro, Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium, R. Handberg, School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK, DenmarkA. Miglio, School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK,
  • T. Arentoft
  • S. Basu, Department of Astronomy, Yale University, New Haven, CT 06520, USA, T. R. Bedding, Sydney Institute for Astronomy, School of Physics, University of Sydney, Sydney, Australia,
  • J. Christensen-Dalsgaard
  • G. R. Davies, School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK, Y. P. Elsworth, School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK, R. L. Gilliland, Center for Exoplanets and Habitable Worlds, The Pennsylvania State University, University Park, PA 16802, USA,
  • C. Karoff
  • S. D. Kawaler, Department of Physics and Astronomy, Iowa State University, Ames, IA 50011, USA,
  • H. Kjeldsen
  • M. Lundkvist
  • T. S. Metcalfe
  • V. Silva Aguirre
  • D. Stello, Sydney Institute for Astronomy, School of Physics, University of Sydney, Sydney, Australia
Original languageEnglish
Article number123
JournalAstrophysical Journal
Volume783
Issue number2
Number of pages17
ISSN0004-637X
DOIs
StatePublished - 1 Mar 2014

    Research areas

  • methods: statistical, planetary systems, stars: late-type, stars: oscillations, techniques: photometric

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ID: 71758650