Distant radio galaxies and their environments
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 …
and the environments in which they are located. HzRGs have several distinct constituents …
Radio and millimeter continuum surveys and their astrophysical implications
G De Zotti, M Massardi, M Negrello, J Wall - The Astronomy and …, 2010 - Springer
We review the statistical properties of the main populations of radio sources, as emerging
from radio and millimeter sky surveys. Recent determinations of local luminosity functions …
from radio and millimeter sky surveys. Recent determinations of local luminosity functions …
Science with ASKAP: The Australian square-kilometre-array pathfinder
The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a
telescope under development by a consortium of 17 countries. The SKA will be 50 times …
telescope under development by a consortium of 17 countries. The SKA will be 50 times …
The second epoch Molonglo Galactic Plane Survey: compact source catalogue
T Murphy, T Mauch, A Green… - Monthly Notices of …, 2007 - academic.oup.com
We present the first data release from the second epoch Molonglo Galactic Plane Survey
(MGPS-2). MGPS-2 was carried out with the Molonglo Observatory Synthesis Telescope at a …
(MGPS-2). MGPS-2 was carried out with the Molonglo Observatory Synthesis Telescope at a …
The star formation history of the Universe as revealed by deep radio observations
N Seymour, T Dwelly, D Moss, I McHardy… - Monthly Notices of …, 2008 - academic.oup.com
Discerning the exact nature of the sub-mJy radio population has been historically difficult
due to the low luminosity of these sources at most wavelengths. Using deep ground based …
due to the low luminosity of these sources at most wavelengths. Using deep ground based …
The 700 ks Chandra Spiderweb Field-II. Evidence for inverse-Compton and thermal diffuse emission in the Spiderweb galaxy
P Tozzi, R Gilli, A Liu, S Borgani, M Lepore… - Astronomy & …, 2022 - aanda.org
Aims. We present the X-ray imaging and spectral analysis of the diffuse emission around the
radio galaxy J1140-2629 (the Spiderweb galaxy) at z= 2.16 and of its nuclear emission …
radio galaxy J1140-2629 (the Spiderweb galaxy) at z= 2.16 and of its nuclear emission …
Extragalactic peaked-spectrum radio sources at low frequencies
We present a sample of 1483 sources that display spectral peaks between 72 MHz and 1.4
GHz, selected from the GaLactic and Extragalactic All-sky Murchison Widefield Array …
GHz, selected from the GaLactic and Extragalactic All-sky Murchison Widefield Array …
Search and analysis of giant radio galaxies with associated nuclei (SAGAN)-I. New sample and multi-wavelength studies
We present the first results of a project called SAGAN, which is dedicated solely to the
studies of relatively rare megaparsec-scale radio galaxies in the Universe, called giant radio …
studies of relatively rare megaparsec-scale radio galaxies in the Universe, called giant radio …
Radio continuum surveys with square kilometre array pathfinders
In the lead-up to the Square Kilometre Array (SKA) project, several next-generation radio
telescopes and upgrades are already being built around the world. These include APERTIF …
telescopes and upgrades are already being built around the world. These include APERTIF …
Why z > 1 radio-loud galaxies are commonly located in protoclusters
Distant powerful radio-loud active galactic nuclei (RLAGN) tend to reside in dense
environments and are commonly found in protoclusters at z> 1.3. We examine whether this …
environments and are commonly found in protoclusters at z> 1.3. We examine whether this …