Early evolution of galaxies and of large-scale structure from CMB experiments. (arXiv:1904.04531v1 [astro-ph.GA])
<a href="http://arxiv.org/find/astro-ph/1/au:+Zotti_G/0/1/0/all/0/1">Gianfranco De Zotti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bonato_M/0/1/0/all/0/1">Matteo Bonato</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Negrello_M/0/1/0/all/0/1">Mattia Negrello</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Herranz_D/0/1/0/all/0/1">Diego Herranz</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lopez_Caniego_M/0/1/0/all/0/1">Marcos Lopez-Caniego</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Trombetti_T/0/1/0/all/0/1">Tiziana Trombetti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Burigana_C/0/1/0/all/0/1">Carlo Burigana</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bonavera_L/0/1/0/all/0/1">Laura Bonavera</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gonzalez_Nuevo_J/0/1/0/all/0/1">Joaquin Gonzalez-Nuevo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hanany_S/0/1/0/all/0/1">Shaul Hanany</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rocha_G/0/1/0/all/0/1">Graca Rocha</a>
Next generation CMB experiments with arcmin resolution will, for free, lay
the foundations for a real breakthrough on the study of the early evolution of
galaxies and galaxy clusters, thanks to the detection of large samples of
strongly gravitationally lensed galaxies and of proto-clusters of dusty
galaxies up to high redshifts. This has an enormous legacy value. High
resolution follow-up of strongly lensed galaxies will allow the direct
investigation of their structure and kinematics up to z~6, providing direct
information on physical processes driving their evolution. Follow-up of
proto-clusters will allow an observational validation of the formation history
of the most massive dark matter halos up to z~4, well beyond the redshift range
accessible via X-ray or SZ measurements. These experiments will also allow a
giant leap forward in the determination of polarization properties of
extragalactic sources, and will provide a complete census of cold dust
available for star formation in the local universe.
Next generation CMB experiments with arcmin resolution will, for free, lay
the foundations for a real breakthrough on the study of the early evolution of
galaxies and galaxy clusters, thanks to the detection of large samples of
strongly gravitationally lensed galaxies and of proto-clusters of dusty
galaxies up to high redshifts. This has an enormous legacy value. High
resolution follow-up of strongly lensed galaxies will allow the direct
investigation of their structure and kinematics up to z~6, providing direct
information on physical processes driving their evolution. Follow-up of
proto-clusters will allow an observational validation of the formation history
of the most massive dark matter halos up to z~4, well beyond the redshift range
accessible via X-ray or SZ measurements. These experiments will also allow a
giant leap forward in the determination of polarization properties of
extragalactic sources, and will provide a complete census of cold dust
available for star formation in the local universe.
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