activity
20052010
most citedThe Star Formation History of the Universe as Revealed by Deep Radio Observations

190 citations · 294 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2010★ 35 cited

Radio and X-ray variability in the Seyfert galaxy NGC 4051

Sadie Jones, Ian McHardy, Derek Moss +5

We present intensive quasi-simultaneous X-ray and radio monitoring of the narrow line Seyfert 1 galaxy NGC 4051, over a 16 month period in 2000-2001. Observations were made with th…

astro-ph2008

The Contribution of Radio Selected Star Forming Galaxies to the IR Energy Density Budget

N. Seymour, T. Dwelly, D. Moss +6

We have used several different methods (radio morphology, radio spectral index, mid-IR to radio and near-IR to radio flux density ratios) to discriminate between AGN and SFGs in fa…

astro-ph2008★ 190 cited

The Star Formation History of the Universe as Revealed by Deep Radio Observations

N. Seymour, T. Dwelly, D. Moss +6

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…

astro-ph2007★ 1 cited

A 610 MHz Survey of the 1H XMM-Newton/Chandra Survey Field

D. Moss, N. Seymour, I. M. McHardy +3

We present the results of a deep 610 MHz survey of the 1^H XMM/Chandra survey area with the GMRT. The resulting maps have a resolution of ~7 arcsec and an rms noise limit of 60 mic…

astro-ph2006

The Star-formation History of the Universe as Revealed from Deep Radio Observations of the 13H XMM-Newton/Chandra Deep Field

N. Seymour, T. Dwelly, D. Moss +4

Discerning the exact nature of the faint (sub-mJy) radio population has been historically difficult due to the low luminosity of these sources at most wavelengths. Using deep obser…

astro-ph2006★ 39 cited

X-ray spectra of sources in the 13H XMM-Newton / Chandra deep field

M. J. Page, N. S. Loaring, T. Dwelly +8

We present the X-ray spectra of 86 optically-identified sources in the 13H XMM-Newton/Chandra deep field which have >70 X-ray counts. The sample consists of 50 broad line AGN, 25 n…