Nuclear Activity is more prevalent in Star-Forming Galaxies
D.J. Rosario, P. Santini, D. Lutz, H. Netzer, F.E. Bauer, S. Berta, B., Magnelli, P. Popesso, D. Alexander, W.N. Brandt, R. Genzel, R. Maiolino, J.R., Mullaney, R. Nordon, A. Saintonge, L. Tacconi, S. Wuyts

TL;DR
This study investigates the relationship between nuclear activity and star formation in galaxies, revealing that low and moderate luminosity AGNs are more commonly found in actively star-forming galaxies, especially those rich in cold gas.
Contribution
It demonstrates that AGNs are preferentially located in star-forming galaxies and highlights the limitations of UV-optical colors as star formation indicators in AGN hosts.
Findings
AGNs are more prevalent in star-forming galaxies
UV-optical colors are poor tracers of star formation in AGN hosts
Cold gas supply influences AGN accretion rates
Abstract
We explore the question of whether low and moderate luminosity Active Galactic Nuclei (AGNs) are preferentially found in galaxies that are undergoing a transition from active star formation to quiescence. This notion has been suggested by studies of the UV-to-optical colors of AGN hosts, which find them to be common among galaxies in the so-called "Green Valley", a region of galaxy color space believed to be composed mostly of galaxies undergoing star-formation quenching. Combining the deepest current X-ray and Herschel. PACS far-infrared (FIR) observations of the two Chandra Deep Fields (CDFs) with redshifts, stellar masses and rest-frame photometry derived from the extensive and uniform multi-wavelength data in these fields, we compare the rest-frame U-V color distributions and SFR distributions of AGNs and carefully constructed samples of inactive control galaxies. The UV-to-optical…
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