activity
20212025
most citedAssessing differences between local galaxy dust attenuation and point source extinction within the same environments

4 citations · 15 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.IM2025

Moonlit sky polarization patterns from Cerro Paranal

B. Pereira, S. Gonzalez-Gaitan, A. M. Mourao +5

We investigate the polarization patterns from the moonlit sky as observed from the European Southern Observatory at Cerro Paranal. The moonlit sky background can be significant in…

astro-ph.GA2025★ 3 cited

Narrow absorption lines from intervening material in supernovae. II. Galaxy properties

Santiago González-Gaitán, Claudia P. Gutiérrez, Gonçalo Martins +11

The interstellar medium (ISM) has a number of tracers such as the Na I D 5890, 5896 AA absorption lines that are evident in the spectra of galaxies but also in those of individual…

astro-ph.GA2025★ 4 cited

Assessing differences between local galaxy dust attenuation and point source extinction within the same environments

J. Duarte, S. González-Gaitán, A. Mourão +5

Dust attenuation in galaxies has often been used as a proxy for the extinction of point sources, such as supernovae, even though this approach ignores fundamental differences betwe…

astro-ph.GA2025★ 3 cited

from multi-waveband galaxy polarimetry in supernovae vicinity

João Rino-Silvestre, Santiago González-Gaitán, Ana Mourão +2

Peculiar dust extinction laws have been reported for some type Ia supernovae (SNe) with the parameter much lower than the average value for the Milky Way (MW) of 3.1. Using o…

astro-ph.IM2022★ 2 cited

Spatial field reconstruction with INLA: Application to simulated galaxies

Majda Smole, João Rino-Silvestre, Santiago González-Gaitán +1

Aims. Monte Carlo Radiative Transfer (MCRT) simulations are a powerful tool for understanding the role of dust in astrophysical systems and its influence on observations. However,…

astro-ph.IM2022★ 3 cited

EmulART: Emulating Radiative Transfer -- A pilot study on autoencoder based dimensionality reduction for radiative transfer models

João Rino-Silvestre, Santiago González-Gaitán, Marko Stalevski +4

Dust is a major component of the interstellar medium. Through scattering, absorption and thermal re-emission, it can profoundly alter astrophysical observations. Models for dust co…