Asteroseismology of solar-type stars with Kepler I: Data analysis
English
Karoff, C.[School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK; Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark]
Chaplin, W. J.[School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK]
Elsworth, Y.[School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK]
Garcia, R.[Université Paris Diderot - Paris 7 > > > >]
Houdek, G.[Institute of Astronomy, University of Vienna, A-1180 Vienna, Austria]
Metcalfe, T. S.[High Altitude Observatory and Scientific Computing Division, National Center for Atmospheric Research, Boulder, CO 80307, USA]
Molenda-Żakowicz, J.[Astronomical Institute, University of Wroclaw, ul. Kopernika, 11, 51-622 Wroclaw, Poland]
Monteiro, M J P F G[Centro de Astrofísica and DFA-Faculdade de Ciências, Universidade do Porto, Ruas das Estrelas, 4150-762 Porto, Portugal]
Thompson, M. J.[School of Mathematics and Statistics, University of Sheffield, Hounsfield Road, Sheffield S3 7RH, UK]
Christensen-Dalsgaard, J.[Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark]
Gilliland, R. L.[Space Telescope Science Institute, Baltimore, MD 21218, USA]
Kjeldsen, H.[Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark]
Basu, S.[Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101, USA]
Bedding, T. R.[Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia]
Campante, T. L.[Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark; Centro de Astrofísica and DFA-Faculdade de Ciências, Universidade do Porto, Ruas das Estrelas, 4150-762 Porto, Portugal]
Eggenberger, P.[Geneva Observatory, University of Geneva, Maillettes 51, 1290 Sauverny, Switzerland]
Fletcher, S. T.[Materials Engineering Research Institute, Faculty of Arts, Computing, Engineering and Sciences, Sheffield Hallam University, Sheffield, S1 1WB, UK]
Mathur, S.[High Altitude Observatory and Scientific Computing Division, National Center for Atmospheric Research, Boulder, CO 80307, USA]
Mosser, B.[LESIA, CNRS, Université Pierre et Marie Curie, Université, Denis Diderot, Observatoire de Paris, 92195 Meudon Cedex, France]
Regulo, C.[Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain; Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain]
Roxburgh, I. W.[Queen Mary University of London, Astronomy Unit, Mile End Road, London E1 4NS, UK]
Salabert, D.[Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain; Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain]
Stello, D.[Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia]
Verner, G. A.[Queen Mary University of London, Astronomy Unit, Mile End Road, London E1 4NS, UK]
Belkacem, Kevin[Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie]
Mathis, S.[Laboratoire AIM, CEA/DSM-CNRS-Université Paris Diderot, IRFU/SAp Centre de Saclay, F-91191 Gif-sur-Yvette, France]
Noels-Grötsch, Arlette[Département d'Astrophysique, Géophysique et Océanographie (AGO), Université de Liége, Allée du 6 Aoüt 17 4000 Liége 1, Belgium]
Noyes, R. W.[Smithsonian Astrophysical Observatory, Cambridge, MA, USA]
Roca Cortes, T.[Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain; Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain]
Roth, M.[Kiepenheuer-Institut für Sonnenphysik, Schöneckstr. 6, 79104 Freiburg, Germany]
Sato, K. H.[Laboratoire AIM, CEA/DSM-CNRS, Université Paris 7 Diderot, IRFU/SAp-SEDI, Centre de Saclay, 91191, Gif-sur-Yvette, France]
Schmitt, J.[Observatoire de Haute-Provence, F-04870, St.Michel l'Observatoire, France]
Suran, M. D.[Astronomical Institute of the Romanian Academy, Str. Cutitul de Argint, 5, RO 40557, Bucharest, Romania]
Trampedach, R.[JILA, University of Colorado, 440 UCB, Boulder, CO 80309-0440, USA]
Uytterhoeven, K.[Laboratoire AIM, CEA/DSM-CNRS, Université Paris 7 Diderot, IRFU/SAp-SEDI, Centre de Saclay, 91191, Gif-sur-Yvette, France]
Ventura, R.[INAF Osservatorio Astrofisico di Catania, Via S. Sofia 78, 95123, Catania, Italy]
[en] We report on the first asteroseismic analysis of solar-type stars observed by Kepler. Observations of three G-type stars, made at one-minute cadence during the first 33.5 days of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: About 20 modes of oscillation can clearly be distinguished in each star. We discuss the appearance of the oscillation spectra, including the presence of a possible signature of faculae, and the presence of mixed modes in one of the three stars.