Radio continuum surveys and galaxy evolution: The AGN view
Vernesa Smolcic (University of Zagreb)
TL;DR
This paper reviews recent advancements in radio continuum sky surveys, highlighting their role in understanding the physical properties and cosmic evolution of radio AGN from early universe to present.
Contribution
It provides an overview of recent developments in radio surveys and their impact on studying galaxy evolution and AGN over cosmic time.
Findings
Radio surveys have significantly advanced understanding of AGN evolution.
Enhanced sensitivity of new facilities enables exploration of galaxies up to z~5.
Radio AGN properties inform models of galaxy formation and evolution.
Abstract
Understanding how galaxies form in the early universe and their subsequent evolution through cosmic time is a major goal of modern astrophysics. Panchromatic look-back sky surveys significantly advanced the field in the past decades, and we are now entering an even more fruitful period - a 'golden age' of radio astronomy - with upgraded, and new facilities delivering an order of magnitude increase in sensitivity. An overview of recent developments in radio continuum sky surveys, focusing on the physical properties and cosmic evolution of radio AGN since z~5 is presented here.
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