2001/02/01 by M. A. Garrett, T. W. B. Muxlow, S. T. Garrington +10 · 1 citation
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Galaxies: Formation, Evolution, Phenomena #High resolution #Hubble Deep Field #Hubble Deep Field South #Hubble Ultra-Deep Field #Maser #Radio Astronomy Observations and Technology #Radio astronomy #Very-long-baseline interferometry #astro-ph
paper · pdf · doi:10.1051/0004-6361:20000537
4 pages, 1 Figure. See http://www.jive.nl/~mag/hdf/evn/pr/ for better quality images/more info. To appear in the "Proceedings of the 5th EVN Symposium", Eds. J. Conway, A. Polatidis, R.Booth., Onsala Space Observatory, Chalmers Technical University, Gothenburg, Sweden (2000)
openalex publication_date 2001/02/01 · arxiv created 2001/02/02 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We present deep, wide-field European VLBI Network (EVN) 1.6 GHz observations of the Hubble Deep Field (HDF) region with a resolution of 0.025 arcseconds. Above the 210 μJy/beam () detection level, the EVN clearly detects two radio sources in a field that encompasses the HDF and part of the Hubble Flanking Fields (HFF). The sources detected are: VLA J123644+621133 (a , low-luminosity FR-I radio source located within the HDF itself) and VLA J123642+621331 (a dust enshrouded, optically faint, starburst system). A third radio source, VLA J123646+621404, is detected at the level. The VLBI detections of all three sources suggest that most of the radio emission of these particular sources (including the dusty starburst) is generated by an embedded AGN.