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Published online by Cambridge University Press: 12 April 2016
Spectroscopic observations of the δ Scuti star V480 Tau, obtained during the MUSICOS 1996 campaign (Hao et al., 2001), detected a large number of modes. In order to assess the information available from such data, we compare the observed spectrum of frequencies with the theoretical predictions obtained for models computed by including the effect of fast rotation on global oscillations.