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Next generation CMB experiments with arcmin resolution will, for free, laythe foundations for a real breakthrough on the study of the early evolution ofgalaxies and galaxy clusters, thanks to the detection of large samples ofstrongly gravitationally lensed galaxies and of proto-clusters of dustygalaxies up to high redshifts. This has an enormous legacy value. Highresolution follow-up of strongly lensed galaxies will allow the directinvestigation of their structure and kinematics up to z~6, providing directinformation on physical processes driving their evolution. Follow-up ofproto-clusters will allow an observational validation of the formation historyof the most massive dark matter halos up to z~4, well beyond the redshift rangeaccessible via X-ray or SZ measurements. These experiments will also allow agiant leap forward in the determination of polarization properties ofextragalactic sources, and will provide a complete census of cold dustavailable for star formation in the local universe.

Early evolution of galaxies and of large-scale structure from CMB experiments