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19992007
most citedA survey of polarization in the JVAS/CLASS flat-spectrum radio source surveys: I. The data and catalogue production

64 citations · 74 across the 5 of their papers we have counts for

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astro-ph200764 cited

A survey of polarization in the JVAS/CLASS flat-spectrum radio source surveys: I. The data and catalogue production

N. Jackson, R. A. Battye, I. W. A. Browne +3

We have used the very large JVAS/CLASS 8.4-GHz surveys of flat-spectrum radio sources to obtain a large, uniformly observed and calibrated, sample of radio source polarizations. Th…

astro-ph20078 cited

CU Virginis - The First Stellar Pulsar

Barry J. Kellett, Vito Graffagnino, Robert Bingham +2

CU Virginis is one of the brightest radio emitting members of the magnetic chemically peculiar (MCP) stars and also one of the fastest rotating. We have now discovered that CU Vir…

astro-ph2006

Sub-arcsecond, microJy radio properties of Spitzer identified mid-infrared sources in the HDF-N/GOODS-N field

R. J. Beswick, T. W. B. Muxlow, H. Thrall +1

We present recent and ongoing results from extremely deep 18 day MERLIN + VLA 1.4GHz observations (rms: 3.3microJy/bm) of an 8.5-by-8.5 arcminute field centred upon the Hubble Deep…

astro-ph2006

High resolution observations of a selection of faint 1.4GHz radio counterparts to optical sources in the HDF-N

H. Thrall, T. W. B. Muxlow, R. J. Beswick +1

We present recent results from very deep MERLIN/VLA 1.4GHz observations of an 8.5-by-8.5 arcminute field centred on the the Hubble Deep Field North, in conjunction with BVIz catalo…

astro-ph2006

The Statistical Properties Of The Very Weak Radio Source Population In The GOODS/ACS HDF-N Region

T. W. B. Muxlow, R. J. Beswick, H. Thrall +3

Deep combination radio observations at 1.4GHz with the VLA and MERLIN have imaged a region 10 arcminutes square surrounding the Hubble Deep Field North (HDF-N). Initial studies of…

astro-ph2006

Starburst Galaxies

T. W. B. Muxlow, R. J. Beswick, A. M. S. Richards +1

Star-formation and the Starburst phenomenon are presented with respect to a number of nearby star-forming galaxies where our understanding of the process can be calibrated. Methods…