Verifying asteroseismically determined parameters of Kepler stars using Hipparcos parallaxes: Self-consistent stellar properties and distances

V. Silva Aguirre*, L. Casagrande, S. Basu, T. L. Campante, W. J. Chaplin, D. Huber, A. Miglio, A. M. Serenelli, J. Ballot, T. R. Bedding, J. Christensen-Dalsgaard, O. L. Creevey, Y. Elsworth, R. A. García, R. L. Gilliland, S. Hekker, H. Kjeldsen, S. Mathur, T. S. Metcalfe, M. J.P.F.G. MonteiroB. Mosser, M. H. Pinsonneault, D. Stello, A. Weiss, P. Tenenbaum, J. D. Twicken, K. Uddin

*Corresponding author for this work

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