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dc.contributor.authorMorganti, R.en_US
dc.contributor.authorGarrett, M. A.en_US
dc.contributor.authorChapman, S.en_US
dc.contributor.authorBaan, W.en_US
dc.contributor.authorHelou, G.en_US
dc.contributor.authorSoifer, T.en_US
dc.date.accessioned2014-03-12T19:20:57Z
dc.date.available2014-03-12T19:20:57Z
dc.date.issued2004-09en_US
dc.identifier.citationMorganti, R., M. A. Garrett, S. Chapman, W. Baan, et al. 2004. "A Deep WSRT 1.4 GHz Radio Survey of the Spitzer Space Telescope FLSv Region." 424(1): 371-378en_US
dc.identifier.issn0004-6361en_US
dc.identifier.urihttp://dx.doi.org/10.1051/0004-6361:20040266en_US
dc.identifier.urihttp://hdl.handle.net/10222/45404
dc.description.abstractThe First Look Survey (FLS) is the first scientific product to emerge from the Spitzer Space Telescope. A small region of this field (the verification strip) has been imaged very deeply, permitting the detection of cosmologically distant sources. We present Westerbork Synthesis Radio Telescope (WSRT) observations of this region, encompassing a ~1 sq. deg field, centred on the verification strip (J2000 RA=17:17:00.00, DEC=59:45:00.000). The radio images reach a noise level of ~ 8.5 microJy/beam - the deepest WSRT image made to date. We summarise here the first results from the project, and present the final mosaic image, together with a list of detected sources. The effect of source confusion on the position, size and flux density of the faintest sources in the source catalogue are also addressed. The results of a serendipitous search for HI emission in the field are also presented. Using a subset of the data, we clearly detect HI emission associated with four galaxies in the central region of the FLSv. These are identified with nearby, massive galaxies.en_US
dc.titleA Deep WSRT 1.4 GHz Radio Survey of the Spitzer Space Telescope FLSv Regionen_US
dc.title.alternativeAstronomy and Astrophysicsen_US
dc.typearticleen_US
dc.identifier.volume424en_US
dc.identifier.issue1en_US
dc.identifier.startpage371en_US
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