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

W.~J. Chaplin, H. Kjeldsen, T.~R. Bedding, J. Christensen-Dalsgaard, R.~L. Gilliland, S.~D. Kawaler, T. Appourchaux, Y. Elsworth, R.~A. García, G. Houdek, C. Karoff, T.~S. Metcalfe, J. Molenda-Zakowicz, M.~J.~P.~F.~G. Monteiro, M.~J. Thompson, G.~A. Verner, N. Batalha, W.~J. Borucki, T.~M. Brown, S.~T. BrysonJ.~L. Christiansen, B.~D. Clarke, J.~M. Jenkins, T.~C. Klaus, D. Koch, D. An, J. Ballot, S. Basu, O. Benomar, A. Bonanno, A.-M. Broomhall, T.~L. Campante, E. Corsaro, O.~L. Creevey, L. Esch, N. Gai, P. Gaulme, S.~J. Hale, R. Handberg, S. Hekker, D. Huber, S. Mathur, B. Mosser, R. New, M.~H. Pinsonneault, D. Pricopi, P.-O. Quirion, C. Régulo, I.~W. Roxburgh, D. Salabert, D. Stello, M.~D. Suran

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