Radio galaxies and feedback from AGN jets
MJ Hardcastle, JH Croston - New Astronomy Reviews, 2020 - Elsevier
We review current understanding of the population of radio galaxies and radio-loud quasars
from an observational perspective, focusing on their large-scale structures and dynamics …
from an observational perspective, focusing on their large-scale structures and dynamics …
Active galactic nuclei: what's in a name?
P Padovani, DM Alexander, RJ Assef… - The Astronomy and …, 2017 - Springer
Active galactic nuclei (AGN) are energetic astrophysical sources powered by accretion onto
supermassive black holes in galaxies, and present unique observational signatures that …
supermassive black holes in galaxies, and present unique observational signatures that …
Host galaxy properties and offset distributions of fast radio bursts: implications for their progenitors
We present observations and detailed characterizations of five new host galaxies of fast
radio bursts (FRBs) discovered with the Australian Square Kilometre Array Pathfinder …
radio bursts (FRBs) discovered with the Australian Square Kilometre Array Pathfinder …
Characterizing the fast radio burst host galaxy population and its connection to transients in the local and extragalactic universe
We present the localization and host galaxies of one repeating and two apparently
nonrepeating fast radio bursts (FRBs). FRB 20180301A was detected and localized with the …
nonrepeating fast radio bursts (FRBs). FRB 20180301A was detected and localized with the …
First results from the IllustrisTNG simulations: the galaxy colour bimodality
D Nelson, A Pillepich, V Springel… - Monthly Notices of …, 2018 - academic.oup.com
We introduce the first two simulations of the IllustrisTNG project, a next generation of
cosmological magnetohydrodynamical simulations, focusing on the optical colours of …
cosmological magnetohydrodynamical simulations, focusing on the optical colours of …
Inferring the star formation histories of massive quiescent galaxies with bagpipes: evidence for multiple quenching mechanisms
AC Carnall, RJ McLure, JS Dunlop… - Monthly Notices of the …, 2018 - academic.oup.com
ABSTRACT We present Bayesian Analysis of Galaxies for Physical Inference and Parameter
EStimation, or bagpipes, a new python tool that can be used to rapidly generate complex …
EStimation, or bagpipes, a new python tool that can be used to rapidly generate complex …
The host galaxies and progenitors of fast radio bursts localized with the Australian Square Kilometre Array Pathfinder
Abstract The Australian SKA Pathfinder (ASKAP) telescope has started to localize fast radio
bursts (FRBs) to arcsecond accuracy from the detection of a single pulse, allowing their host …
bursts (FRBs) to arcsecond accuracy from the detection of a single pulse, allowing their host …
The star formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics
M Donnari, A Pillepich, D Nelson… - Monthly Notices of …, 2019 - academic.oup.com
We select galaxies from the IllustrisTNG hydrodynamical simulations (at 0≤ z≤ 2) and
characterize the shapes and evolutions of their UVJ and star formation rate–stellar mass …
characterize the shapes and evolutions of their UVJ and star formation rate–stellar mass …
Introducing the Illustris project: the evolution of galaxy populations across cosmic time
We present an overview of galaxy evolution across cosmic time in the Illustris simulation.
Illustris is an N-body/hydrodynamical simulation that evolves 2× 18203 resolution elements …
Illustris is an N-body/hydrodynamical simulation that evolves 2× 18203 resolution elements …
Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing
M Donnari, A Pillepich, GD Joshi… - Monthly Notices of …, 2021 - academic.oup.com
We use the IllustrisTNG hydrodynamical simulations to show how the fractions of quenched
galaxies vary across different environments and cosmic time, and to quantify the role AGN …
galaxies vary across different environments and cosmic time, and to quantify the role AGN …