A numerous population of weak line galaxies (WLGs) is often left out of statistical studies on
emission-line galaxies (ELGs) due to the absence of an adequate classification scheme …

We studied the global and local ℳ-Z relation based on the first data available from the
CALIFA survey (150 galaxies). This survey provides integral field spectroscopy of the …

We have studied the radial structure of the stellar mass surface density (μ∗) and stellar
population age as a function of the total stellar mass and morphology for a sample of 107 …

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 …

Gas-phase metallicities of galaxies are typically measured through auroral or nebular
emission lines, but metallicity also leaves an imprint on the overall spectral energy …

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 …

We present the stellar surface mass density versus gas metallicity (Σ*-Z) relation for more
than 500 000 spatially resolved star-forming resolution elements (spaxels) from a sample of …

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 …

We demonstrate the existence of a local mass, metallicity, star formation relation using
spatially resolved optical spectroscopy of H ii regions in the local universe. One of the …