Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies. (arXiv:2206.15286v1 [astro-ph.CO])
<a href="http://arxiv.org/find/astro-ph/1/au:+Magliocchetti_M/0/1/0/all/0/1">Manuela Magliocchetti</a>

Despite their relative sparseness, during the recent years it has become more
and more clear that extragalactic radio sources (both AGN and star-forming
galaxies) constitute an extremely interesting mix of populations, not only
because of their intrinsic value, but also for their fundamental role in
shaping our Universe the way we see it today. Indeed, radio-active AGN are now
thought to be the main players involved in the evolution of massive galaxies
and clusters. At the same time, thanks to the possibility of being observed up
to very high redshifts, radio galaxies can also provide crucial information on
both the star-formation history of our Universe and on its Large-Scale
Structure properties and their evolution. In the light of present and
forthcoming facilities such as LOFAR, MeerKAT and SKA that will probe the radio
sky to unprecedented depths and widths, this review aims at providing the
current state of the art on our knowledge of extragalactic radio sources in
connection with their hosts, large-scale environments and cosmological context.

Despite their relative sparseness, during the recent years it has become more
and more clear that extragalactic radio sources (both AGN and star-forming
galaxies) constitute an extremely interesting mix of populations, not only
because of their intrinsic value, but also for their fundamental role in
shaping our Universe the way we see it today. Indeed, radio-active AGN are now
thought to be the main players involved in the evolution of massive galaxies
and clusters. At the same time, thanks to the possibility of being observed up
to very high redshifts, radio galaxies can also provide crucial information on
both the star-formation history of our Universe and on its Large-Scale
Structure properties and their evolution. In the light of present and
forthcoming facilities such as LOFAR, MeerKAT and SKA that will probe the radio
sky to unprecedented depths and widths, this review aims at providing the
current state of the art on our knowledge of extragalactic radio sources in
connection with their hosts, large-scale environments and cosmological context.

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