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20062020
most citedThe faint source population at 15.7 GHz - I. The radio properties

37 citations · 110 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2020★ 6 cited

The faint radio source population at 15.7 GHz -- IV. The dominance of core emission in faint radio galaxies

I. H. Whittam, D. A. Green, M. J. Jarvis +1

We present 15-GHz Karl G. Jansky Very Large Array observations of a complete sample of radio galaxies selected at 15.7 GHz from the Tenth Cambridge (10C) survey. 67 out of the 95 s…

astro-ph.GA2016★ 19 cited

10C continued: a deeper radio survey at 15.7 GHz

I. H. Whittam, J. M. Riley, D. A. Green +5

We present deep 15.7-GHz observations made with the Arcminute Microkelvin Imager Large Array in two fields previously observed as part of the Tenth Cambridge (10C) survey. These ob…

astro-ph.GA2015★ 14 cited

The faint radio source population at 15.7 GHz - II. Multi-wavelength properties

I. H. Whittam, J. M. Riley, D. A. Green +2

A complete, flux density limited sample of 96 faint ( mJy) radio sources is selected from the 10C survey at 15.7 GHz in the Lockman Hole. We have matched this sample to a ra…

astro-ph.CO2012★ 37 cited

The faint source population at 15.7 GHz - I. The radio properties

I. H. Whittam, J. M. Riley, D. A. Green +6

We have studied a sample of 296 faint (> 0.5 mJy) radio sources selected from an area of the Tenth Cambridge (10C) survey at 15.7 GHz in the Lockman Hole. By matching this catalogu…

astro-ph.CO2010★ 14 cited

Further GMRT observations of the Lockman Hole at 610 MHz

T. S. Garn, D. A. Green, J. M. Riley +1

We present further observations of the Lockman Hole field, made with the Giant Metrewave Radio Telescope at 610 MHz with a resolution of 6 x 5 arcsec^2. These complement our earlie…

astro-ph.CO2009★ 14 cited

High-redshift obscured quasars: radio emission at sub-kiloparsec scales

H. -R. Kloeckner, A. Martinez-Sansigre, S. Rawlings +1

The radio properties of 11 obscured `radio-intermediate' quasars at redshifts z>~2 have been investigated using the European Very-Long-Baseline-Interferometry Network (EVN) at 1.66…