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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★ 2 cited
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}…