The cold interstellar medium (ISM) plays a central role in the galaxy evolution process. It is
the reservoir that fuels galaxy growth via star formation, the repository of material formed by …

We study the presence of optically-selected active galactic nuclei (AGNs) within a sample of
867 galaxies extracted from the extended Calar-Alto Legacy Integral Field spectroscopy …

We investigate the nature of the scaling relations between the surface density of star
formation rate (ΣSFR), stellar mass (Σ*), and molecular gas mass (), aiming at distinguishing …

Feedback from an active galactic nucleus (AGN) is often implicated as a mechanism that
leads to the quenching of galactic star formation. However, AGN-driven quenching is …

Abstract The ALMaQUEST (ALMA-MaNGA QUEnching and STar formation) survey is a
program with spatially resolved 12 CO (1− 0) measurements obtained with the Atacama …

Context. In this work we study the stellar mass–metallicity relation (MZR) of an extended
sample of star-forming galaxies in the local Universe and its possible dependence on the …

We present a new characterization of the relations between star-formation rate, stellar mass,
and molecular gas mass surface densities at different spatial scales across galaxies (from …

I review the spatially resolved spectroscopic properties of low-redshift star-forming galaxies
(and their retired counterparts) using results from the most recent optical integral field …

Context. Energy and momentum injected by young, massive stars into the surrounding gas
play an important role in regulating further star formation and in determining the galaxy's …

This paper describes the extended data release (eDR) of the Calar Alto Legacy Integral
Field Area (CALIFA) survey. It comprises science-grade quality data for 895 galaxies …