We apply the spectral energy distribution (SED) fitting code ProSpect to multiwavelength
imaging for∼ 7000 galaxies from the GAMA survey at z< 0.06, in order to extract their star …

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 use direct method oxygen abundances in combination with strong optical emission lines,
stellar masses (M⋆), and star formation rates (SFRs) to recalibrate the N2, O3N2, and N2O2 …

A recent multiyear Caltech-NRAO Stripe 82 Survey revealed a group of objects that
appeared as new radio sources after> 5–20 yr of absence. They are transient phenomena …

We study the galactic wind in the edge-on spiral galaxy UGC 10043 with the combination of
the CALIFA integral field spectroscopy data, scanning Fabry–Perot interferometry (FPI) and …

We introduce the data analysis pipeline (DAP) for the Sloan Digital Sky Survey V Local
Volume Mapper (LVM) project, referred to as the LVM-DAP. We outline our methods for …

The origin of the low-ionization nuclear emission-line region (LINER) prevalent in local
galaxies and its relationship with supermassive black holes have been debated for decades …

Integrated light spectroscopy from galaxies can be used to study the stellar populations that
cannot be resolved into individual stars. This analysis relies on stellar population synthesis …

We study the conditions for the onset of thermal instability in the innermost regions of
compact galactic nuclei, where the properties of the interstellar environment are governed …

We present a study on the stellar populations and stellar ages of a subsample of far-infrared
(FIR) active galactic nucleus (AGN) and non-AGN green valley galaxies at using the data …