collaborators

8 papers

astro-ph.GA2026

Nebular continuum in high-redshift galaxies with JWST

Henrique Miranda, Ciro Pappalardo, José Afonso +2

Studying the relevance of accounting for both stellar and nebular continuum emission when performing optical spectral fitting has been mainly limited to galaxies in the local Unive…

astro-ph.GA2026

The Road to Identifying the Earliest Radio-Powerful AGN with the SKA

Jose Afonso, Stergios Amarantidis, Stas Shabala +20

The Epoch of Reionization (EoR) is one of the most pivotal frontiers in modern astrophysics, marking the emergence of the first galaxies, stars, and supermassive black holes (SMBHs…

astro-ph.GA2026

EMU/GAMA: A statistical perspective on active galactic nuclei diagnostics

J. Prathap, A. M. Hopkins, R. Carvajal +19

While it is well known that galaxies are composites of many emission processes, quantifying the various contributions remains challenging. In this work, we use unsupervised machine…

astro-ph.GA2025

ALMA reveals diverse dust-to-gas mass ratios and quenching modes in old quiescent galaxies

Giuliano Lorenzon, Darko Donevski, Allison W. S. Man +18

Recent discoveries of dust and molecular gas in quiescent galaxies (QGs) up to challenge the long-standing view that the interstellar medium depletes rapidly once star for…

astro-ph.GA2025

Importance of modelling the nebular continuum in galaxy spectra

Henrique Miranda, Ciro Pappalardo, José Afonso +7

The neglect of modelling both stellar and nebular emission significantly affects the derived physical properties of galaxies, particularly those with high star formation rates. Whi…

astro-ph.GA2025

Unveiling faint X-ray AGN populations in the NewAthena era: Insights from cosmological simulations

Nuno Covas, Israel Matute, Stergios Amarantidis +7

Recent observations expanded our understanding of galaxy formation and evolution, yet key challenges persist in the X-ray regime, crucial for studying Active Galactic Nuclei (AGN).…