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The VLA-COSMOS Survey. IV. Deep Data and Joint Catalog

Schinnerer, E. and Sargent, M. T. and Bondi, M. and Smolčić , V. and Datta, A. and Carilli, C. L. and Bertoldi, F. and Blain, A. and Ciliegi, P. and Koekemoer, A. and Scoville, N. Z. (2010) The VLA-COSMOS Survey. IV. Deep Data and Joint Catalog. Astrophysical Journal Supplement Series, 188 (2). pp. 384-404. ISSN 0067-0049. http://resolver.caltech.edu/CaltechAUTHORS:20100709-110106023

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Abstract

In the context of the VLA-COSMOS Deep project, additional VLA A array observations at 1.4 GHz were obtained for the central degree of the COSMOS field and combined with the existing data from the VLA-COSMOS Large project. A newly constructed Deep mosaic with a resolution of 2".5 was used to search for sources down to 4σ with 1σ ≈ 12 μJy beam^(–1) in the central 50' × 50'. This new catalog is combined with the catalog from the Large project (obtained at 1".5 × 1".4 resolution) to construct a new Joint catalog. All sources listed in the new Joint catalog have peak flux densities of ≥5σ at 1".5 and/or 2".5 resolution to account for the fact that a significant fraction of sources at these low flux levels are expected to be slightly resolved at 1".5 resolution. All properties listed in the Joint catalog, such as peak flux density, integrated flux density, and source size, are determined in the 2".5 resolution Deep image. In addition, the Joint catalog contains 43 newly identified multi-component sources.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0067-0049/188/2/384DOIArticle
http://iopscience.iop.org/0067-0049/188/2/384PublisherArticle
ORCID:
AuthorORCID
Schinnerer, E.0000-0002-3933-7677
Scoville, N. Z.0000-0002-0438-3323
Additional Information:© 2010 American Astronomical Society. Received 2008 December 19; accepted 2010 April 19; published 2010 May 17. The National Radio Astronomy Observatory (NRAO) is operated by Associated Universities, Inc., under cooperative agreement with the National Science Foundation. We thank the NRAOfor their support during this project.We thank our referee Jim Condon for his insightful comments for improving the paper. C.C. thanks the Max-Planck-Gesellschaft and the Humboldt-Stiftung for support through the Max-Planck-Forschungspreis. C.C. and A.D. acknowledge support through NASA grant HST-GO-09822.33-A. M.T.S. acknowledges support by the German DFG under grant SCHI 536/3-2 and SCHI 536/3-3. V.S. acknowledges support by the German DFG under grant SCHI 536/3-1. This project has been (partially) funded by the DFG Priority Programme 1177 “Galaxy Evolution.”
Group:COSMOS, Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
National Radio Astronomy ObservatoryUNSPECIFIED
Max-Planck-ForschungspreisUNSPECIFIED
NASAHST-GO-09822.33-A
Deutsche Forschungsgemeinschaft (DFG)SCHI 536/3-2
Deutsche Forschungsgemeinschaft (DFG)SCHI 536/3-3
Deutsche Forschungsgemeinschaft (DFG)SCHI 536/3-1
Deutsche Forschungsgemeinschaft (DFG)Priority Programme 1177 “Galaxy Evolution”
Subject Keywords:cosmology: observations; radio continuum: galaxies; surveys
Classification Code:PACS: 95.80.+p; 98.80.-k; 98.54.Cm; 98.70.Dk
Record Number:CaltechAUTHORS:20100709-110106023
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20100709-110106023
Official Citation:E. Schinnerer et al 2010 ApJS 188 384 doi: 10.1088/0067-0049/188/2/384
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:18963
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:09 Jul 2010 19:56
Last Modified:18 May 2017 22:29

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