Filippo Mannucci

TL;DR: In this paper, the authors provide an overview of the methods used to constrain the chemical enrichment in galaxies and their environment, and discuss the observed scaling relations between metallicity and galaxy properties, the observed relative chemical abundances, how the chemical elements are distributed within galaxies, and how these properties evolve across the cosmic epochs.

TL;DR: In this paper, the authors provide an overview of the methods used to constrain the chemical enrichment in galaxies and their environment, and discuss the observed scaling relations between metallicity and galaxy properties, the observed relative chemical abundances, how the chemical elements are distributed within galaxies, and how these properties evolve across the cosmic epochs.

TL;DR: In this paper, the authors acknowledge financial support from INAF and the Italian Ministry of University and Research under the contracts PRIN-INAF-2011 (“Black Hole growth and AGN feedback through cosmic time”) and PRIN MIUR 2010-2011(“The dark Universe and the cosmic evolution of baryons”).

TL;DR: The WISSH quasars project has been designed to reveal the most energetic AGN-driven outflows, estimate their occurrence at the peak of quasar activity, and extend the study of correlations between outflows and nuclear properties up to poorly investigated, extreme AGN luminosities as discussed by the authors.

TL;DR: In this article, the authors reported the results of their ongoing search for extincted supernovae (SNe) at near-infrared wavelengths, and measured a SN rate of SN NIR = 7:6 3:8 SNu which is an order of magnitude larger than observed in quiescent galaxies.