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Asteroseismology of solar-type stars with Kepler: III. Ground-based data

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dc.contributor.authorMolenda-Zakowicz, Jen_AU
dc.contributor.authorBruntt, Hen_AU
dc.contributor.authorSousa, Sen_AU
dc.contributor.authorFrasca, Aen_AU
dc.contributor.authorBiazzo, Ken_AU
dc.contributor.authorHuber, Den_AU
dc.contributor.authorBedding, Timothy Russellen_AU
dc.contributor.authorStello, Dennisen_AU
dc.contributor.authorUytterhoeven, Ken_AU
dc.contributor.authorDreizler, Sen_AU
dc.contributor.authorIreland, Michaelen_AU
dc.date.accessioned2015-12-10T23:23:16Z
dc.date.issued2010
dc.date.updated2016-02-24T09:59:26Z
dc.description.abstractWe report on the ground-based follow-up program of spectroscopic and photometric observations of solar-like asteroseismic targets for the Kepler space mission. These stars constitute a large group of more than a thousand objects which are the subject of an intensive study by the Kepler Asteroseismic Science Consortium Working Group 1 (KASC WG-1). In the current work we will discuss the methods we use to determine the fundamental stellar atmospheric parameters using high-quality stellar spectra. These provide essential constraints for the asteroseismic modelling and make it possible to verify the parameters in the Kepler Input Catalogue (KIC).
dc.identifier.issn0004-6337
dc.identifier.urihttp://hdl.handle.net/1885/66878
dc.publisherWiley-VCH Verlag GMBH
dc.sourceAstronomische Nachrichten
dc.subjectKeywords: Space vehicles; Stars: fundamental parameters; Stars: oscillations
dc.titleAsteroseismology of solar-type stars with Kepler: III. Ground-based data
dc.typeJournal article
local.bibliographicCitation.issue9-10
local.bibliographicCitation.lastpage984
local.bibliographicCitation.startpage981
local.contributor.affiliationMolenda-Zakowicz, J, University of Wrocław
local.contributor.affiliationBruntt, H, Observatoire de Paris-Meudon
local.contributor.affiliationSousa, S, Universidade do Porto
local.contributor.affiliationFrasca, A, INAF-Osservatorio Astrofisicio di Catania
local.contributor.affiliationBiazzo, K, INAF-Osservatorio Astrofisicio di Arcetri
local.contributor.affiliationHuber, D, University of Sydney
local.contributor.affiliationIreland, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBedding, Timothy Russell , University of Sydney
local.contributor.affiliationStello, Dennis, University of Sydney
local.contributor.affiliationUytterhoeven, K, CEA/DSM-CNRS-Universite Paris Diderot
local.contributor.affiliationDreizler, S, Georg-August Universitat
local.contributor.authoruidIreland, Michael, u5544212
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationU3488905xPUB1360
local.identifier.citationvolume331
local.identifier.doi10.1002/asna.201011440
local.identifier.scopusID2-s2.0-78649440774
local.identifier.thomsonID000285211700025
local.type.statusPublished Version

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