Morphological number counts and redshift distributions to I< 26 from the hubble deep field: Implications for the evolution of ellipticals, spirals, and irregulars

S. P. Driver, A. Fernández-Soto, W. J. Couch, S. C. Odewahn, Rogier Windhorst, S. Phillipps, K. Lanzetta, A. Yahil

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