Establishing the accuracy of asteroseismic mass and radius estimates of giant stars. I. Three eclipsing systems at [Fe/H]~ -0.3 and the need for a large high-precision sample

K. Brogaard, C. J. Hansen, A. Miglio, D. Slumstrup, S. Frandsen, J. Jessen-Hansen, M. N. Lund, D. Bossini, A. Thygesen, G. R. Davies, W. J. Chaplin, T. Arentoft, H. Bruntt, F. Grundahl, R. Handberg

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