activity
20102024
most citedThe faint source population at 15.7 GHz - I. The radio properties

37 citations · 105 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2024★ 1 cited

Brightening and Fading in the Youngest Galactic Supernova Remnant G1.9+0.3: 13 years of monitoring with the Chandra X-ray Observatory

Kazimierz J. Borkowski, Stephen P. Reynolds, Robert Petre +1

We report results from 13 years of Chandra monitoring of nonthermal X-ray emission from the youngest Galactic supernova remnant G1.9+0.3, the only remnant known to be increasing in…

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.GA2018★ 13 cited

Constraining the nature of DG Tau A's thermal and non-thermal radio emission

S. J. D. Purser, R. E. Ainsworth, T. P. Ray +3

DG Tau A, a class-II young stellar object (YSO) displays both thermal, and non-thermal, radio emission associated with its bipolar jet. To investigate the nature of this emission,…

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.HE2013★ 1 cited

A combined GMRT/CLFST image of IC443 at 150 MHz

D. Mitra, D. A. Green, A. Pramesh Rao

IC443 is a relatively large Galactic (~45 arcmin) SNR with a high radio surface brightness. It has fine scale structure down to arcsec scales, and so is difficult to image on all a…