Galaxy evaluation from multi-colour surveys
The number density and clustering evolution of massive galaxies, particularly at redshift <I>z </I>> 1, can be used to place strong constraints on galaxy evolution models. On the one hand passive evolution models predict a constant comoving density of massive galaxies to high redshift...
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University of Cambridge
2002
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.599033 |