output
20142023
most citedAccretion mode versus radio morphology in the LOFAR Deep Fields

66 citations

8 papers

astro-ph.GA2023★ 18 cited

Radio spectral properties of star-forming galaxies between 150-5000MHz in the ELAIS-N1 field

Fangxia An, M. Vaccari, P. N. Best +9

By combining high-sensitivity LOFAR 150MHz, uGMRT 400MHz and 1,250MHz, GMRT 610MHz, and VLA 5GHz data in the ELAIS-N1 field, we study the radio spectral properties of radio-detecte…

physics.soc-ph2022

The ASIMOV Prize for scientific publishing -- HEP researchers trigger young people toward science

Andrea Ventura, Wanda Maria Alberico, Roberta Antolini +28

This work presents the ASIMOV Prize for scientific publishing, which was launched in Italy in 2016. The prize aims to bring the young generations closer to scientific culture, thro…

astro-ph.GA2022★ 39 cited

Identifying active galactic nuclei via brightness temperature with sub-arcsecond International LOFAR Telescope observations

Leah K. Morabito, F. Sweijen, J. F. Radcliffe +11

Identifying active galactic nuclei (AGN) and isolating their contribution to a galaxy's energy budget is crucial for studying the co-evolution of AGN and their host galaxies. Brigh…

astro-ph.GA2022★ 52 cited

Cosmic evolution of low-excitation radio galaxies in the LOFAR Two-meter Sky Survey Deep Fields

R. Kondapally, P. N. Best, R. K. Cochrane +16

Feedback from low-excitation radio galaxies (LERGs) plays a key role in the lifecycle of massive galaxies in the local Universe; their evolution, and the impact of these active gal…

astro-ph.GA2022★ 66 cited

Accretion mode versus radio morphology in the LOFAR Deep Fields

B. Mingo, J. H. Croston, P. N. Best +17

Radio-loud active galaxies have two accretion modes [radiatively inefficient (RI) and radiatively efficient (RE)], with distinct optical and infrared signatures, and two jet dynami…

astro-ph.GA2022★ 19 cited

The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the -SFR relation

Michael Romano, L. Morselli, P. Cassata +22

The [CII] 158m emission line represents so far one of the most profitable tools for the investigation of the high-redshift galaxies in the early Universe. Being one of the brig…