Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies

M Magliocchetti - The Astronomy and Astrophysics Review, 2022 - Springer
Despite their relative sparseness, during the recent years it has become more and more
clear that extragalactic radio sources (both AGN and star-forming galaxies) constitute an …

Fitting AGN/Galaxy X-Ray-to-radio SEDs with CIGALE and Improvement of the Code

G Yang, M Boquien, WN Brandt, V Buat… - The Astrophysical …, 2022 - iopscience.iop.org
Modern and future surveys effectively provide a panchromatic view for large numbers of
extragalactic objects. Consistently modeling these multiwavelength survey data is a critical …

MIGHTEE: total intensity radio continuum imaging and the COSMOS/XMM-LSS Early Science fields

I Heywood, MJ Jarvis, CL Hale… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT MIGHTEE is a galaxy evolution survey using simultaneous radio continuum,
spectropolarimetry, and spectral line observations from the South African MeerKAT …

The hidden side of cosmic star formation at z> 3-Bridging optically dark and Lyman-break galaxies with GOODS-ALMA

MY **ao, D Elbaz, C Gómez-Guijarro, L Leroy… - Astronomy & …, 2023 - aanda.org
Our current understanding of the cosmic star formation history at z> 3 is primarily based on
UV-selected galaxies (Lyman-break galaxies, ie, LBGs). Recent studies of H-dropouts (HST …

MIGHTEE: the nature of the radio-loud AGN population

IH Whittam, MJ Jarvis, CL Hale… - Monthly Notices of …, 2022 - academic.oup.com
We study the nature of the faint radio source population detected in the MeerKAT
International GHz Tiered Extragalactic Exploration (MIGHTEE) Early Science data in the …

MIGHTEE: deep 1.4 GHz source counts and the sky temperature contribution of star-forming galaxies and active galactic nuclei

CL Hale, IH Whittam, MJ Jarvis, PN Best… - Monthly Notices of …, 2023 - academic.oup.com
We present deep 1.4 GHz source counts from∼ 5 deg2 of the continuum Early Science data
release of the MeerKAT International Gigahertz Tiered Extragalactic Exploration survey …

Diagnosing deceivingly cold dusty galaxies at 3.5< z< 6: A substantial population of compact starbursts with high infrared optical depths

S **, E Daddi, GE Magdis, D Liu, JR Weaver… - Astronomy & …, 2022 - aanda.org
Using NOEMA and ALMA 3mm line scans, we measured spectroscopic redshifts of six new
dusty galaxies at 3.5< z< 4.2 by solidly detecting [CI](1-0) and CO transitions. The sample …

A New Estimate of the Cosmic Star Formation Density from a Radio-selected Sample, and the Contribution of H-dark Galaxies at z≥ 3

A Enia, M Talia, F Pozzi, A Cimatti… - The Astrophysical …, 2022 - iopscience.iop.org
The star formation rate density (SFRD) history of the universe is well constrained up to
redshift z∼ 2. At earlier cosmic epochs, the picture has been largely inferred from UV …

The evolving interstellar medium of star-forming galaxies, as traced by stardust

VI Kokorev, GE Magdis, I Davidzon… - The Astrophysical …, 2021 - iopscience.iop.org
We analyze the far-infrared (FIR) properties of∼ 5000 star-forming galaxies at z< 4.5, drawn
from the deepest, super-deblended catalogs in the GOODS-N and COSMOS fields. We …

How does the radio enhancement of broad absorption line quasars relate to colour and accretion rate?

JW Petley, LK Morabito, AL Rankine… - Monthly Notices of …, 2024 - academic.oup.com
The origin of radio emission in different populations of radio-quiet quasars is relatively
unknown, but recent work has uncovered various drivers of increased radio-detection …