activity
20242026
collaborators

5 papers

astro-ph.GA2026

Opening new parameter space windows on galaxy/AGN co-evolution with SKA radio continuum surveys

Isabella Prandoni, Mark T. Sargent, Matteo Bonato +11

In this chapter we provide an overview of the science enabled by the SKAO, focusing on galaxy/AGN co-evolution studies. In particular we discuss a number of radio continuum `refere…

astro-ph.GA2025

How accurately can obscured galaxy luminosities be measured using spectral energy distribution fitting of near- through far-infrared observations?

Duncan Farrah, Kiana Ejercito, Andreas Efstathiou +23

Infrared-luminous galaxies are important sites of stellar and black hole mass assembly at most redshifts. Their luminosities are often estimated by fitting spectral energy distribu…

astro-ph.GA2025

Host galaxy identification of LOFAR sources in the Euclid Deep Field North

Bisigello L., Giulietti M., Prandoni I. +6

We present a catalogue of optical and near-infrared counterparts to radio sources detected in the Euclid Deep Field North (EDF-N) using observations from the LOw-Frequency ARray (L…

astro-ph.GA2025

Sub-arcsecond-resolution LOFAR observations of bright sub-millimetre galaxies in the North Ecliptic Pole field

M. Bondi, I. Prandoni, M. Magliocchetti +6

Bright SMGs contribute significantly to the star formation rate (SFR) density (20-50\%) and stellar mass density ( 30-50\%) at 2-4 with SFRs M,yr$^{-1}…

astro-ph.GA2024

A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution

Matteo Bonato, David Leisawitz, Gianfranco De Zotti +10

Far-infrared (FIR) surveys are critical to probing the co-evolution of black holes and galaxies, since of order half the light from accreting black holes and active star formation…