activity
20102023
most citedThe VISTA Deep Extragalactic Observations (VIDEO) Survey

349 citations · 1.4k across the 19 of their papers we have counts for

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Showing astro-ph.COShow all

6 papers · 1 filter

astro-ph.CO2014★ 29 cited

Evolution in the bias of faint radio sources to z ~ 2.2

S. N. Lindsay, M. J. Jarvis, K. McAlpine

Quantifying how the baryonic matter traces the underlying dark matter distribution is key to both understanding galaxy formation and our ability to constrain the cosmological model…

astro-ph.CO2013★ 67 cited

Evolution of faint radio sources in the VIDEO-XMM3 field

K. McAlpine, M. J. Jarvis, D. G. Bonfield

It has been speculated that low luminosity radio-loud AGN have the potential to serve as an important source of AGN feedback, and may be responsible for suppressing star-formation…

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.CO2012★ 349 cited

The VISTA Deep Extragalactic Observations (VIDEO) Survey

Matt J. Jarvis, D. G. Bonfield, V. A. Bruce +25

In this paper we describe the first data release of the the Visible and Infrared Survey Telescope for Astronomy (VISTA) Deep Extragalactic Observations (VIDEO) survey. VIDEO is a ~…

astro-ph.CO2012★ 31 cited

Impact of Redshift Information on Cosmological Applications with Next-Generation Radio Surveys

Stefano Camera, Mário G. Santos, David J. Bacon +5

In this paper, we explore how the forthcoming generation of large-scale radio continuum surveys, with the inclusion of some degree of redshift information, can constrain cosmologic…

astro-ph.CO2010★ 17 cited

The evolution of radio sources in the UKIDSS-DXS XMM-LSS field

Kim McAlpine, Matt J. Jarvis

We investigate the cosmic evolution of low luminosity () radio sources in the XMM Large Scale Structure survey field (XMM-LSS). We mat…