collaborators

7 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.GA2025

Through the fog: a complementary optical galaxy classification scheme for 'intermediate' redshifts

Duarte Muñoz Santos, Cirino Pappalardo, Henrique Miranda +10

Understanding galaxy classification depends on our interpretation of their spectra. To date, the hydrogen Balmer lines remain the most consistent way to classify galaxies, but at '…

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).…

astro-ph.GA2025

EMU/GAMA: A new approach to characterising radio luminosity functions

J. Prathap, A. M. Hopkins, J. Afonso +16

This study characterises the radio luminosity functions (RLFs) for SFGs and AGN using statistical redshift estimation in the absence of comprehensive spectroscopic data. Sensitive…