Predicting the Detectability of Oscillations in Solar-type Stars Observed by Kepler - Archive ouverte HAL Accéder directement au contenu
Article Dans Une Revue The Astrophysical Journal Année : 2011

Predicting the Detectability of Oscillations in Solar-type Stars Observed by Kepler

1 School of Physics and Astronomy, University of Birmingham
2 DASC - Danish AsteroSeismology Centre
3 SIfA - Sydney Institute for Astronomy
4 STSci - Space Telescope Science Institute
5 Department of Physics and Astronomy, Iowa State University
6 IAS - Institut d'astrophysique spatiale
7 CEA - Commissariat à l'énergie atomique et aux énergies alternatives
8 IfA - Institut für Astronomie, Universität Wien
9 High Altitude Observatory, National Center for Atmospheric Research
10 Astronomical Institute, University of Wroclaw
11 Universidade do Porto = University of Porto
12 National Aeronautics and Space Administration, Ames Research Center
13 Las Cumbres Observatory, Goleta
14 SETI Institute, NASA Ames Research Center, Moffett Field
15 Orbital Sciences Corporation, NASA Ames Research Center, Moffett Field
16 Department of Science Education, Ewha Womans University
17 IRAP - Institut de recherche en astrophysique et planétologie
18 Department of Astronomy, Yale University
19 INAF-OACt - INAF-Osservatorio Astrofisico di Catania
20 ULL - Universidad de La Laguna [Tenerife - SP]
21 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique
22 Etoile
23 Materials Engineering Research Institute, Faculty of Arts, Computing, Engineering and Sciences, Sheffield Hallam University
24 Department of Astronomy, Ohio State University
25 Astronomical Institute of the Romanian Academy, Bucharest
26 CSA - Canadian Space Agency
27 IAC - Instituto de Astrofisica de Canarias
28 School of Mathematical Sciences, Queen Mary Unversity of London

Résumé

Asteroseismology of solar-type stars has an important part to play in the exoplanet program of the NASA Kepler Mission. Precise and accurate inferences on the stellar properties that are made possible by the seismic data allow very tight constraints to be placed on the exoplanetary systems. Here, we outline how to make an estimate of the detectability of solar-like oscillations in any given Kepler target, using rough estimates of the temperature and radius, and the Kepler apparent magnitude.

Dates et versions

hal-03785510 , version 1 (23-09-2022)

Identifiants

Citer

William J. Chaplin, Hans Kjeldsen, Timothy R. Bedding, Jörgen Christensen-Dalsgaard, Ronald L. Gilliland, et al.. Predicting the Detectability of Oscillations in Solar-type Stars Observed by Kepler. The Astrophysical Journal, 2011, 732, pp.54. ⟨10.1088/0004-637X/732/1/54⟩. ⟨hal-03785510⟩
21 Consultations
0 Téléchargements

Altmetric

Partager

Gmail Mastodon Facebook X LinkedIn More