papers

Publications (12)

astro-ph.GA2021

An ACA 1mm survey of HzRGs in the ELAIS-S1: survey description and first results

Hugo Messias, Evanthia Hatziminaoglou, Pascale Hibon +16

Radio-emitting jets might be one of the main ingredients shaping the evolution of massive galaxies in the Universe since early cosmic times. However, identifying early radio active…

astro-ph.GA2021

Self-consistent population spectral synthesis with FADO: II. Star formation history of galaxies in spectral synthesis methods

Ciro Pappalardo, Leandro S. M. Cardoso, Jean Michel Gomes +12

The field of galaxy evolution will make a great leap forward in the next decade as a consequence of the huge effort by the scientific community in multi-object spectroscopic facili…

astro-ph.GA2017

ELDAR, a new method to identify AGN in multi-filter surveys: the ALHAMBRA test-case

Jonás Chaves-Montero, Silvia Bonoli, Mara Salvato +15

We present ELDAR, a new method that exploits the potential of medium- and narrow-band filter surveys to securely identify active galactic nuclei (AGN) and determine their redshifts…

astro-ph.GA2019

The first Super Massive Black Holes: indications from models for future observations

Stergios Amarantidis, José Afonso, Hugo Messias +12

We present an exploration of the expected detection of the earliest Active Galactic Nuclei (AGN) in the Universe from state-of-art galaxy formation and evolution semi-analytic mode…

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

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…