Properties of 42 solar-type Kepler targets from the asteroseismic modeling portal

T. S. Metcalfe*, O. L. Creevey, Gülnur Dogan, S. Mathur, H. Xu, T. R. Bedding, W. J. Chaplin, J. Christensen-Dalsgaard, C. Karoff, R. Trampedach, O. Benomar, B. P. Brown, D. L. Buzasi, T. L. Campante, Z. Çelik, M. S. Cunha, G. R. Davies, S. Deheuvels, A. Derekas, M. P Di MauroR. A. García, J. A. Guzik, R. Howe, K. B. Macgregor, A. Mazumdar, J. Montalbán, M. J P F G Monteiro, D. Salabert, A. Serenelli, D. Stello, M. Stęs̈licki, M. D. Suran, M. Yildiz, C. Aksoy, Y. Elsworth, M. Gruberbauer, D. B. Guenther, Y. Lebreton, K. Molaverdikhani, D. Pricopi, R. Simoniello, T. R. White

*Corresponding author for this work

Research output: Contribution to journal/Conference contribution in journal/Contribution to newspaperJournal articleResearchpeer-review

1 Citation (Scopus)
Original languageEnglish
Article number27
JournalAstrophysical Journal Supplement Series
Volume214
Issue2
Number of pages13
ISSN0067-0049
DOIs
Publication statusPublished - 2014

Keywords

  • methods: numerical
  • stars: evolution
  • stars: interiors
  • stars: oscillations

Cite this