We review the use of emission lines for understanding galaxy evolution, focusing on
excitation source, metallicity, ionization parameter, ISM pressure, and electron density. We …

We present the characterization of the main properties of a sample of 98 AGN host galaxies,
both type-II and type-I, in comparison with those of≈ 2700 non-active galaxies observed by …

We investigated the interstellar medium (ISM) properties of the disc and outflowing gas in
the central regions of nine nearby Seyfert galaxies, all characterised by prominent conical or …

We compute synthetic, rest-frame optical and ultraviolet (UV) emission-line properties of
galaxy populations at redshifts from z≈ 0 to= 8 in a full cosmological framework. We achieve …

We use spatially resolved spectroscopy from the Calar Alto Legacy Integral Field Area
(CALIFA) survey to study the nature of the line emitting gas in galaxies of different Hubble …

We present HOMERUN (Highly Optimized Multi-cloud Emission-line Ratios Using photo-
ionizatioN), a new approach to modeling emission lines from photoionized gas that can …

We present an updated version of the mass–metallicity (MZ) relation using integral field
spectroscopy data obtained from 734 galaxies observed by the CALIFA survey. These …

We measured gas-phase metallicity, ionisation parameter, and dust extinction for a
representative sample of 1795 local star-forming galaxies using integral field spectroscopy …

We present a detailed exploration of the stellar mass versus gas-phase metallicity relation
(MZR) using integral field spectroscopy data obtained from∼ 1000 galaxies observed by the …

We present the results of the archaeological analysis of the stellar populations of a sample
of∼ 4000 galaxies observed by the SDSS-IV MaNGA survey using pipe3d. Based on this …