activity
20242026
collaborators

6 papers

astro-ph.CO2026

Local luminosity functions of galaxies at (sub)millimeter wavelengths from Planck surveys

Matteo Bonato, Gianfranco De Zotti

The Planck all-sky surveys at (sub)millimeter wavelengths enable us to accurately determine the corresponding local luminosity functions up to the highest luminosities. The detecte…

astro-ph.GA2026

A pilot sample of Planck-selected strongly lensed sub-mm galaxies: NOEMA observations and physical characterisation

Leonardo Trobbiani, Matteo Bonato, Ivano Baronchelli +6

The extreme brightness of high- strongly lensed galaxies detected by Planck surveys, thanks to their exceptionally large gravitational magnifications, offers a unique opportunit…

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

The dust emissivity index beta in infrared-bright galaxies at 1.5 < z < 4.2

G. J. Bendo, T. J. L. C. Bakx, H. S. B. Algera +16

We have measured the dust emissivity index beta for 21 infrared-bright sources (including several gravitationally lensed galaxies) at 1.5 < z < 4.2 using Atacama Large Millimeter/s…

astro-ph.GA2025

Using Planck maps for a systematic search of ultra-bright high-redshift strongly lensed galaxies

Matteo Bonato, Leonardo Trobbiani, Ivano Baronchelli +6

This paper presents a novel approach to the use of Planck telescope data for the systematic search of ultra-bright high-redshift strongly lensed galaxies. These galaxies provide cr…

astro-ph.GA2024

A Novel high-z submm Galaxy Efficient Line Survey in ALMA bands 3 through 8 -- An ANGELS Pilot

T. J. L. C. Bakx, A. Amvrosiadis, G. J. Bendo +32

We use the Atacama Large sub/Millimetre Array (ALMA) to efficiently observe spectral lines across Bands 3, 4, 5, 6, 7, and 8 at high-resolution (0.5" - 0.1") for 16 bright southern…