VLBI images of Lockman Hole radio sources Virtual Observatory Resource

Authors
  1. Middelberg, E.
  2. Deller, A.
  3. Norris, R.
  4. Fotopuoulou, S.
  5. Salvato, M.
  6. Morgan, J.
  7. Brisken, W.
  8. Lutz, D.
  9. Rovilos, E.
  10. Published by
    The GAVO DC team
Abstract
 These are 1.4GHz Very Long Baseline Interferometry images of 532
radio sources with a flux density exceeding 100uJy as determined by
Ibar et al. (2009, MNRAS, 397, 281), obtained between 2010-06-03 and
2010-09-03.

For all fields, we give frames processed using natural weighting to
preserve maximal sensitivity. For the 65 detected sources, we
additionally give frames processed using uniform weighting to suppress
sidelobes (see Middelberg et al. 2013, A&A 551, 97 for details) in
flux density measurements. Some sources have larger images to cover a
larger area because the initial coordinates were not sufficiently
accurate.
Keywords
  1. radio-interferometry
  2. galaxy-evolution
  3. active-galaxies
Bibliographic source Bibcode
2013A&A...551A..97M
See also HTML
http://dc.zah.uni-heidelberg.de/emi/q/s/info
IVOA Identifier IVOID
ivo://org.gavo.dc/emi/q/s
Document Object Identifer DOI

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History

2013-04-09T12:57:26Z
Resource record created
2024-01-16T16:41:20Z
updated

Contact

Name
GAVO Data Center Team
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