SIMBAD references

We present deep, wide-field European VLBI Network (EVN) 1.6GHz observations of the Hubble Deep Field (HDF) region with a resolution of 0.025 arcseconds. Above the 210µJy/beam (5σ) 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 z=1.013, low-luminosity FR-I radio source located within the HDF itself) and VLA J123642+621331 (a dust enshrouded, optically faint, z=4.424 starburst system). A third radio source, VLA J123646+621404, is detected at the 4σ 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.