Reference : Ground-based follow-up in relation to Kepler asteroseismic investigation
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/110807
Ground-based follow-up in relation to Kepler asteroseismic investigation
English
Uytterhoeven, K. [Lab. AIM, CEA/DSM-CNRS-Université Paris Diderot; CEA, IRFU, SAp, Saclay, 91191, Gif-sur-Yvette, France]
Briquet, Maryline mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie]
Bruntt, H. [LESIA, Observatoire de Paris-Meudon, 92195 Meudon, France]
De Cat, P. [Royal Observatory of Belgium, Ringlaan 3, 1180 Brussel, Belgium]
Frandsen, S. [Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark]
Gutiérrez-Soto, J. [Instituto de Astrofísica de Andalucía (CSIC), Apartado 3004, 18080 Granada, Spain]
Kiss, L. [Konkoly Observatory of the Hungarian Academy of Sciences, 1121 Budapest, Hungary; Sydney Institute for Astrophysics, School of Physics, University of Sydney, Australia]
Kurtz, D. W. [Jeremiah Horrocks Institute of Astrophysics, University of Central Lancashire, Preston PR1 2HE, UK]
Marconi, M. [INAF - Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy]
Molenda-Żakowicz, J. [Instytut Astronomiczny, Uniwersytet Wrocławski, Kopernika 11, 51-622 Wrocław, Poland]
Østensen, R. [Instituut voor Sterrenkunde, KULeuven, Celestijnenlaan 200D, 3001 Leuven, Belgium]
Randall, S. [European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany]
Southworth, J. [Department of Physics, University of Warwick, Coventry CV4 7AL, UK]
Szabó, R. [Konkoly Observatory of the Hungarian Academy of Sciences, 1121 Budapest, Hungary]
1-Dec-2010
Astronomische Nachrichten
Wiley
331
993
Yes (verified by ORBi)
International
0004-6337
1521-3994
Berlin
Germany
[en] stars: fundamental parameters ; stars: oscillations ; techniques: photometric ; techniques: spectroscopic
[en] The Kepler space mission, successfully launched in March 2009, is providing continuous and high-precision photometry of thousands of stars simultaneously. The uninterrupted time-series of stars of all known pulsation types are a precious source for asteroseismic studies. The Kepler data do not provide information on the physical parameters, such as T_eff, log g, metallicity, and v sin i, which are crucial for successful asteroseismic modelling. Additional ground-based time-series data are needed to characterize mode parameters in several types of pulsating stars. Therefore, ground-based multi-colour photometry and mid/high-resolution spectroscopy are needed to complement the space data. We present ground-based activities within KASC on selected asteroseismic Kepler targets of several pulsation types. Based on observations made with the Isaac Newton Telescope and William Herschel Telescope operated by the Isaac Newton Group, with the Nordic Optical Telescope, operated jointly by Denmark, Finland, Iceland, Norway, and Sweden, with the Italian Telescopio Nazionale Galileo (TNG) operated by the Fundación Galileo Galilei of the INAF (Istituto Nazionale di Astrofisica), and with the Mercator telescope, operated by the Flemish Community, all on the island of La Palma at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias (IAC). Based on observations made with the IAC-80 operated on the island of Tenerife by the IAC at the Spanish Observatorio del Teide. Also based on observations taken at the observatories of Sierra Nevada, San Pedro Mártir, Vienna, Xinglong, Apache Point, Lulin, Tautenburg, McDonald, Skinakas, Pic du Midi, Mauna Kea, Steward Observatory, Mt. Wilson, Białków Observatory of the Wrocław University, Piszkésteto Mountain Station, and Observatoire de Haute Provence. Based on spectra taken at the Loiano (INAF - OA Bologna), Serra La Nave (INAF - OA Catania) and Asiago (INAF - OA Padova) observatories. Also based on observations collected at the Centro Astronómico Hispano Alemán (CAHA) at Calar Alto, operated jointly by the Max-Planck-Institut für Astronomie and the Instituto de Astrofísica de Andalucía (CSIC). We acknowledge with thanks the variable star observations from the AAVSO International Database contributed by observers worldwide and used in this research. Funding for the Kepler mission is provided by NASA's Science Mission Directorate. We thank the entire Kepler team for the development and operations of this outstanding mission.
http://hdl.handle.net/2268/110807
10.1002/asna.201011444
http://esoads.eso.org/abs/2010AN....331..993U
http://de.arxiv.org/abs/1003.6093

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