2006/12/04 by H. Thrall, Thrall, H., T. W. B. Muxlow +6
Engineering · Physics and Astronomy · #Adaptive optics and wavefront sensing #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #GNSS positioning and interference #Radio Astronomy Observations and Technology #Superconducting and THz Device Technology #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0612076
4 pages, 3 figures, To appear in the proceedings of 'At the Edge of the Universe' (9-13 October 2006, Sintra, Portugal)
arxiv created 2006/12/04 · openalex publication_date 2006/12/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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 catalogues of GOODS/ACS sources detected in this field. In an extension of work by Muxlow et al. (also presented at this conference) on the statistical properties of over 8000 sources, the results presented here take advantage of the deep (rms: 3.3 microJy/bm), sub-arcsecond radio imaging of this field to characterise the properties at 1.4GHz of a number of individual radio counterparts to GOODS/ACS sources.