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Date and Time of the Query: 2019-06-26 T08:10:15 PDT
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For refcode 2000ApJS..131...95F:
Retrieve 374 NED objects in this reference.
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NED Abstract

Copyright by American Astronomical Society. Reproduced by permission
2000ApJS..131...95F The VSOP 5 GHz Continuum Survey: The Prelaunch VLBA Observations E. B. Fomalont National Radio Astronomy Observatory, Charlottesville, VA 22903 S. Frey and Z. Paragi FVMI Satellite Geodetic Observatory, P.O. Box 546, H-1373 Budapest, Hungary L. I. Gurvits Joint Institute for VLBI in Europe, P.O. Box 2, 7990 AA, Dwingeloo, Netherlands W. K. Scott and A. R. Taylor Physics and Astronomy Department, University of Calgary, 2500 University Drive NW, Calgary, Alberta, Canada T2N 1N4 and P. G. Edwards and H. Hirabayashi Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan Received 2000 April 12; accepted 2000 May 16 ABSTRACT We have imaged with milliarcsecond resolution at 5 GHz 374 strong flat- spectrum radio sources north of declination -440 using the VLBA in 1996 June. The source sample was compiled from the source list for the VLBI Space Observatory Programme (VSOP) Survey Program. About 250 of the sources observed with the VLBA had correlated flux densities >=0.3 Jy on the longest VLBA baseline and these sources are currently being observed with VSOP at 5 GHz. This paper presents the results from the VLBA prelaunch observations: the correlated flux density dependence with u-v distance; the contour display of the images; the model fit parameters for each radio component; and improved positions for 62 sources. Comparisons and extensive cross-referencing with other major VLBI surveys are also given. Subject headings: galaxies: active-radio continuum: galaxies -surveys
Retrieve 374 NED objects in this reference.
Please click here for ADS abstract

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