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000002276 005__ 20160701171702.0
000002276 0247_ $$2DOI$$a10.1002/asna.201011440
000002276 037__ $$aASTROimport-433
000002276 100__ $$aMolenda-Zakowicz, J.
000002276 245__ $$aAsteroseismology of solar-type stars with Kepler: III. Ground-based data
000002276 260__ $$c2010
000002276 520__ $$aWe report on the ground-based follow-up program of spectroscopic and photometric observations of solar-like asteroseismic targets for the Kepler space mission. These stars constitute a large group of more than a thousand objects which are the subject of an intensive study by the Kepler Asteroseismic Science Consortium Working Group 1 (KASC WG-1). In the current work we will discuss the methods we use to determine the fundamental stellar atmospheric parameters using high-quality stellar spectra. These provide essential constraints for the asteroseismic modelling and make it possible to verify the parameters in the Kepler Input Catalogue (KIC). 
000002276 700__ $$a Bruntt, H.
000002276 700__ $$a Sousa, S.
000002276 700__ $$a Frasca, A.
000002276 700__ $$a Biazzo, K.
000002276 700__ $$a Huber, D.
000002276 700__ $$a Ireland, M.
000002276 700__ $$a Bedding, T.
000002276 700__ $$a Stello, D.
000002276 700__ $$a Uytterhoeven, K.
000002276 700__ $$a Dreizler, S.
000002276 700__ $$a De Cat, P.
000002276 700__ $$a Briquet, M.
000002276 700__ $$a Catanzaro, G.
000002276 700__ $$a Karoff, C.
000002276 700__ $$a Frandsen, S.
000002276 700__ $$a Spezzi, L.
000002276 773__ $$c981$$i9/10$$pAstronomische Nachrichten$$v331$$y2010
000002276 85642 $$ahttp://esoads.eso.org/abs/2010AN....331..981M
000002276 905__ $$apublished in
000002276 980__ $$aREFERD