A VLBI and MERLIN Survey of faint, compact radio sources
S. T. Garrington, M. A. Garrett, A. G. Polatidis, Macclesfield Sk Dl
Abstract
S. T. Garrington, M. A. Garrett, A. G. Polatidis, Macclesfield Sk Dl
Abstract
We present preliminary results from a VLBI survey at $\\lambda=6 $cm of a sample of 35 sources with flux densities of 2 - 100 mJy. These sources were selected from the VLA FIRST survey at $\\lambda = 20 $cm, in a 3 degree field around the bright calibrator 1156+295, simply by imposing $S_{20} > 10 $ mJy and $\\theta < 5$ arcsec. MERLIN observations at $\\lambda 6 $cm detected 70/127 of these sources with a threshold of 2 mJy at 50 mas resolution and the closest 35 of these to the calibrator were observed with the VLBA+EVN in snapshot mode at $\\lambda 6 $cm. These sources are a mixture of flat and steep-spectrum sources and include: weak flat-spectrum nuclei of large radio galaxies, low power AGN in nearby galaxies and radio quiet quasars. With these short observations, the sensitivity is limited and most appear as either core-jets or simple point sources on the milliarcsec scale. Nonetheless, it is encouraging that with only 10 minutes observation per source, at least 35% of all sources with $S_{20} > 10 $ mJy can be detected and imaged with global 6cm VLBI.
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We present preliminary results from a VLBI survey at $\\lambda=6 $cm of a sample of 35 sources with flux densities of 2 - 100 mJy. These sources were selected from the VLA FIRST survey at $\\lambda = 20 $cm, in a 3 degree field around the bright calibrator 1156+295, simply by imposing $S_{20} > 10 $ mJy and $\\theta < 5$ arcsec. MERLIN observations at $\\lambda 6 $cm detected 70/127 of these sources with a threshold of 2 mJy at 50 mas resolution and the closest 35 of these to the calibrator were observed with the VLBA+EVN in snapshot mode at $\\lambda 6 $cm. These sources are a mixture of flat and steep-spectrum sources and include: weak flat-spectrum nuclei of large radio galaxies, low power AGN in nearby galaxies and radio quiet quasars. With these short observations, the sensitivity is limited and most appear as either core-jets or simple point sources on the milliarcsec scale. Nonetheless, it is encouraging that with only 10 minutes observation per source, at least 35% of all sources with $S_{20} > 10 $ mJy can be detected and imaged with global 6cm VLBI.
Key concepts: Physics, Very-long-baseline interferometry, Astrophysics, Merlin (protein), Astronomy, Galaxy, Quasar, Radio galaxy