activity
20112019
most citedAGN feedback works both ways

110 citations · 463 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.IM2019★ 22 cited

A Comparison of Photometric Redshift Techniques for Large Radio Surveys

Ray P. Norris, M. Salvato, G. Longo +14

Future radio surveys will generate catalogues of tens of millions of radio sources, for which redshift estimates will be essential to achieve many of the science goals. However, sp…

astro-ph.CO2013★ 110 cited

AGN feedback works both ways

Peter-Christian Zinn, Enno Middelberg, Ray P. Norris +1

Simulations of galaxy growth need to invoke strong negative feedback from active galactic nuclei (AGN) to suppress the formation of stars and thus prevent the over-production of ve…

astro-ph.CO2012★ 101 cited

Radio Continuum Surveys with Square Kilometre Array Pathfinders

Ray P. Norris, J. Afonso, D. Bacon +48

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 (T…

astro-ph.IM2012★ 26 cited

Finding New High-Redshift Quasars by Asking the Neighbours

Kai Lars Polsterer, Peter-Christian Zinn, Fabian Gieseke

Quasars with a high redshift (z) are important to understand the evolution processes of galaxies in the early universe. However only a few of these distant objects are known to thi…

astro-ph.CO2012★ 7 cited

X-ray stacking of Lyman break galaxies in the 4\,Ms CDF-S - X-ray luminosities and star formation rates across cosmic time

Peter-Christian Zinn, Stefan Blex, Nicholas Seymour +1

Lyman Break Galaxies (LBGs) are widely thought to be prototypical young galaxies in the early universe, particularly representative of those undergoing massive events of star forma…

astro-ph.CO2012★ 51 cited

The Australia Telescope Large Area Survey: Spectroscopic Catalogue and Radio Luminosity Functions

Minnie Y. Mao, Rob Sharp, Ray P. Norris +9

The Australia Telescope Large Area Survey (ATLAS) has surveyed seven square degrees of sky around the Chandra Deep Field South (CDFS) and the European Large Area ISO Survey - South…

astro-ph.CO2012★ 24 cited

The Australia Telescope Large Area Survey: 2.3 GHz observations of ELAIS-S1 and CDF-S

Peter-Christian Zinn, Enno Middelberg, Ray P. Norris +3

Context. The Australia Telescope Large Area Survey (ATLAS) aims to image a 7 deg2 region centred on the European Large Area ISO Survey - South 1 (ELAIS-S1) field and the Chandra De…

astro-ph.CO2012★ 53 cited

Spectral index properties of milliJansky radio sources

Kate Randall, Andrew Hopkins, Ray Norris +4

At the faintest radio flux densities (S_1.4 < 10 mJy), conflicting results have arisen regarding whether there is a flattening of the average spectral index between a low radio fre…

astro-ph.CO2011★ 13 cited

Supernovae without host galaxies? The low surface brightness host of SN 2009Z

P. -C. Zinn, M. Stritzinger, J. Braithwaite +5

A remarkable fraction of supernovae (SNe) have no obvious host galaxy. Two possible explanations are that (i) the host galaxy is simply not detected within the sensitivity of the a…

astro-ph.CO2011★ 13 cited

Supernovae without host galaxy? - Hypervelocity stars in foreign galaxies

Peter-Christian Zinn, Philipp Grunden, Dominik J. Bomans

Harvesting the SAI supernova catalog, we search for SNe that apparently do not occur within a distinct host galaxy but lie a great distance apart from their assigned host galaxy. A…

astro-ph.IM2011★ 17 cited

Detecting Quasars in Large-Scale Astronomical Surveys

Fabian Gieseke, Kai Lars Polsterer, Andreas Thom +5

We present a classification-based approach to identify quasi-stellar radio sources (quasars) in the Sloan Digital Sky Survey and evaluate its performance on a manually labeled trai…

astro-ph.CO2011★ 26 cited

Infrared-Faint Radio Sources: A Cosmological View - AGN Number Counts, the Cosmic X-Ray Background and SMBH Formation

Peter-Christian Zinn, Enno Middelberg, Edo Ibar

Context. Infrared Faint Radio Sources (IFRS) are extragalactic emitters clearly detected at radio wavelengths but barely detected or undetected at optical and infrared wavelengths,…