Distant radio galaxies and their environments

G Miley, C De Breuck - The Astronomy and Astrophysics Review, 2008 - Springer
We review the properties and nature of luminous high-redshift radio galaxies (HzRGs, z> 2)
and the environments in which they are located. HzRGs have several distinct constituents …

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 …

Mid-infrared selection of active galactic nuclei with the wide-field infrared survey explorer. i. characterizing wise-selected active galactic nuclei in cosmos

D Stern, RJ Assef, DJ Benford, A Blain… - The Astrophysical …, 2012 - iopscience.iop.org
ABSTRACT The Wide-field Infrared Survey Explorer (WISE) is an extremely capable and
efficient black hole finder. We present a simple mid-infrared color criterion, W1− W2⩾ 0.8 …

Identifying luminous active galactic nuclei in deep surveys: revised IRAC selection criteria

JL Donley, AM Koekemoer, M Brusa… - The Astrophysical …, 2012 - iopscience.iop.org
Spitzer/IRAC selection is a powerful tool for identifying luminous active galactic nuclei
(AGNs). For deep IRAC data, however, the AGN selection wedges currently in use are …

The Spitzer–WISE Survey of the Ecliptic Poles

TH Jarrett, M Cohen, F Masci, E Wright… - The Astrophysical …, 2011 - iopscience.iop.org
We have carried out a survey of the north and south ecliptic poles, EP-N and EP-S,
respectively, with the Spitzer Space Telescope and the Wide-field Infrared Survey Explorer …

First results from the JWST Early Release Science Program Q3D: Turbulent times in the life of az∼ 3 extremely red quasar revealed by NIRSpec IFU

D Wylezalek, A Vayner, DSN Rupke… - The Astrophysical …, 2022 - iopscience.iop.org
Extremely red quasars, with bolometric luminosities exceeding 10 47 erg s− 1, are a
fascinating high-redshift population that is absent in the local universe. They are the best …

Bright [C II] and dust emission in three z> 6.6 quasar host galaxies observed by ALMA

BP Venemans, F Walter, L Zschaechner… - The Astrophysical …, 2015 - iopscience.iop.org
We present ALMA detections of the [C ii] 158 μm emission line and the underlying far-
infrared (FIR) continuum of three quasars at 6.6< z< 6.9 selected from the VIKING survey …

A 158 μm [C II] line survey of galaxies at z∼ 1–2: an indicator of star formation in the early universe

GJ Stacey, S Hailey-Dunsheath… - The Astrophysical …, 2010 - iopscience.iop.org
We have detected the 158 μm [C ii] line from 12 galaxies at z∼ 1–2. This is the first survey of
this important star formation tracer at redshifts covering the epoch of maximum star formation …

Driving outflows with relativistic jets and the dependence of active galactic nucleus feedback efficiency on interstellar medium inhomogeneity

AY Wagner, GV Bicknell… - The Astrophysical …, 2012 - iopscience.iop.org
We examine the detailed physics of the feedback mechanism by relativistic active galactic
nucleus (AGN) jets interacting with a two-phase fractal interstellar medium (ISM) in the kpc …

What are protoclusters?–Defining high-redshift galaxy clusters and protoclusters

SI Muldrew, NA Hatch, EA Cooke - Monthly Notices of the Royal …, 2015 - academic.oup.com
We explore the structures of protoclusters and their relationship with high-redshift clusters
using the Millennium Simulation combined with a semi-analytic model. We find that …