A. Gil de Paz

TL;DR: Pipe3D as discussed by the authors is an analysis pipeline based on the FIT3D fitting tool to explore the properties of the stellar populations and ionized gas of Integral Field Spectroscopy data.

TL;DR: In this paper, a detailed study of the spatial variation of the far-infrared (FIR) [C II]158 μm and [O I]63 μm lines and midinfrared H2 emission lines as tracers of gas cooling, and of the polycyclic aromatic hydrocarbon (PAH) bands as tracer of the photoelectric heating, using Herschel-PACS and Spitzer-IRS infrared spectral maps.

TL;DR: In this article, the relation between the outer-disk ionized-gas metallicity gradients and the presence of breaks in the surface brightness profiles of disk galaxies was studied. But the results were limited to the case of low-and high-mass galaxies.

TL;DR: In this paper, the authors investigate the possible origin of the strong radial gradient in the ultraviolet-to-infrared ratio in the nearby late-type spiral galaxy NGC 300 and emphasize the importance of local variations in the geometry of the interstellar medium, concluding that they cannot be neglected with respect to metallicity effects.

TL;DR: In this article, an analysis of the full bidimensional optical spectral cube of the nearby spiral galaxy NGC 5668, observed with the Pmas fiber PAcK Integral Field Unit (IFU) at the Calar Alto observatory 3.5 m telescope, is presented.