VLBI images of Lockman Hole radio sources

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.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/org.gavo.dc/emi/q/s
Related Identifier http://dc.zah.uni-heidelberg.de/emi/q/s/info
Related Identifier http://dc.zah.uni-heidelberg.de/emi/q/browse/form
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://org.gavo.dc/emi/q/s
Provenance
Creator Middelberg, E.; Deller, A.; Norris, R.; Fotopuoulou, S.; Salvato, M.; Morgan, J.; Brisken, W.; Lutz, D.; Rovilos, E.
Publisher The GAVO DC team
Publication Year 2013
OpenAccess true
Contact GAVO Data Center Team <gavo(at)ari.uni-heidelberg.de>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics
Temporal Coverage 2010-07-04T00:00:00Z 2010-07-04T00:00:00Z