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

SP Driver^*, A Fernandez-Soto, WJ Couch, SC Odewahn, RA Windhorst, S Phillipps, K Lanzetta, A Yahil

^*Corresponding author for this work

Research output: Contribution to journal › Article (Academic Journal) › peer-review

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