activity
19972020
most citedSpectral evidence for a powerful compact jet from XTE J1118+480

97 citations · 416 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2020★ 41 cited

LeMMINGs. II. The e-MERLIN legacy survey of nearby galaxies. The deepest radio view of the Palomar sample on parsec scale

R. D. Baldi, D. R. A. Williams, I. M. McHardy +30

We present the second data release of high-resolution ( arcsec) 1.5-GHz radio images of 177 nearby galaxies from the Palomar sample, observed with the e-MERLIN array, as p…

astro-ph.IM2014★ 9 cited

Future mmVLBI Research with ALMA: A European vision

R. P. J. Tilanus, T. P. Krichbaum, J. A. Zensus +165

Very long baseline interferometry at millimetre/submillimetre wavelengths (mmVLBI) offers the highest achievable spatial resolution at any wavelength in astronomy. The anticipated…

astro-ph.HE2013★ 26 cited

Radio and X-ray observations of jet ejection in Cygnus X-2

R. E. Spencer, A. P. Rushton, M. Balucinska-Church +5

The ejection of a relativistic jet has been observed in the luminous Galactic low mass X-ray binary Cygnus X-2. Using high resolution radio observations, a directly resolved ejecti…

astro-ph.GA2009★ 22 cited

A decade of high-resolution radio observations of GRS 1915+105

A. Rushton, R. E. Spencer, G. Pooley +1

The radio emitting X-ray binary GRS 1915+105 shows a wide variety of X-ray and radio states. We present a decade of monitoring observations, with the RXTE-ASM and the Ryle Telescop…

astro-ph2006★ 15 cited

First e-VLBI observations of GRS 1915+105

A. Rushton, R. E. Spencer, M. Strong +10

We present results from the first successful open call e-VLBI science run, observing the X-ray binary GRS 1915+105. e-VLBI science allows the rapid production of VLBI radio maps, w…

astro-ph2005★ 15 cited

Structure in the radio counterpart to the 2004 Dec 27 giant flare from SGR 1806-20

R. P. Fender, T. W. B. Muxlow, M. A. Garrett +7

On Dec 27, 2004, the magnetar SGR 1806-20 underwent an enormous outburst resulting in the formation of an expanding, moving, and fading radio source. We report observations of this…