Abstract
Rich clusters of galaxies and QSO absorption line systems provide two alternative venues for studying the evolution of galaxies at high redshift. Here I review some recent observational results in both areas of investigation, and consider their implications for the history of galaxy evolution since z∼1.
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Dickinson, M. (1996). Galaxy evolution from cluster and absorption-selected samples. In: Martínez-González, E., Sanz, J.L. (eds) The Universe at High-z, Large-Scale Structure and the Cosmic Microwave Background. Lecture Notes in Physics, vol 470. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0102577
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DOI: https://doi.org/10.1007/BFb0102577
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