The VSOP 5 GHz Active Galactic Nucleus Survey. V. Imaging Results for the Remaining 140 Sources
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Citation R. Dodson et al 2008 ApJS 175 314DOI 10.1086/525025
R. Dodson
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
Observatorio Astronómico Nacional, Apartado 112, E-28803, Alcala de Henares, Spain
E. B. Fomalont
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National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903
K. Wiik
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
Tuorla Observatory, University of Turku, Väisäläntie 20, FIN-21500 Piikkiö, Finland
S. Horiuchi
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National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, P.O. Box 218, Hawthorn, Vic. 3122, Australia
Canberra Deep Space Communication Complex, P.O. Box 1035, Tuggeranong, ACT 2901, Australia
H. Hirabayashi
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
Department of Space and Astronautical Science, School of Physical Sciences, The Graduate University for Advanced Studies, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
P. G. Edwards
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
Australia Telescope National Facility, Commonwealth Scientific and Industrial Research Organization, P. O. Box 76, Epping NSW 2122, Australia
Y. Murata
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
Department of Space and Astronautical Science, School of Physical Sciences, The Graduate University for Advanced Studies, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
Y. Asaki
AFFILIATIONS
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
Department of Space and Astronautical Science, School of Physical Sciences, The Graduate University for Advanced Studies, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
G. A. Moellenbrock
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
National Radio Astronomy Observatory, P.O. Box 0, Socorro, NM 87801
W. K. Scott
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Physics and Astronomy Department, University of Calgary, 2500 University Dr. NW, Calgary, AB T2N 1N4, Canada
A. R. Taylor
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Physics and Astronomy Department, University of Calgary, 2500 University Dr. NW, Calgary, AB T2N 1N4, Canada
L. I. Gurvits
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Joint Institute for VLBI in Europe, P.O. Box 2, 7990 AA, Dwingeloo, Netherlands
Z. Paragi
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Joint Institute for VLBI in Europe, P.O. Box 2, 7990 AA, Dwingeloo, Netherlands
MTA Research Group for Physical Geodesy and Geodynamics, P.O. Box 91, H-1521 Budapest, Hungary
S. Frey
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MTA Research Group for Physical Geodesy and Geodynamics, P.O. Box 91, H-1521 Budapest, Hungary
FÖMI Satellite Geodetic Observatory, P.O. Box 585, H-1592, Budapest, Hungary
Z.-Q. Shen
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Lu, Shanghai 200030, China
J. E. J. Lovell
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Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan
Australia Telescope National Facility, Commonwealth Scientific and Industrial Research Organization, P. O. Box 76, Epping NSW 2122, Australia
School of Mathematics and Physics, University of Tasmania, Private Bag 21, Hobart, Australia
S. J. Tingay
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Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, P.O. Box 218, Hawthorn, Vic. 3122, Australia
Department of Imaging and Applied Physics, Curtin University of Technology, Perth, Australia
M. J. Rioja
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Observatorio Astronómico Nacional, Apartado 112, E-28803, Alcala de Henares, Spain
S. Fodor
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Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109
Physics Department, Whittier College, 13406 East Philadelphia, P.O. Box 634, Whittier, CA 90608-4413
M. L. Lister
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Department of Physics, Purdue University, West Lafayette, IN 47907
L. Mosoni
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FÖMI Satellite Geodetic Observatory, P.O. Box 585, H-1592, Budapest, Hungary
MTA Konkoly Observatory, P.O. Box 67, H-1525, Budapest, Hungary
G. Coldwell
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Observatorio Astronómico de la Universidad Nacional de Córdoba, Argentina
B. G. Piner
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Physics Department, Whittier College, 13406 East Philadelphia, P.O. Box 634, Whittier, CA 90608-4413
J. Yang
AFFILIATIONS
Joint Institute for VLBI in Europe, P.O. Box 2, 7990 AA, Dwingeloo, Netherlands
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Lu, Shanghai 200030, China
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Dates
- Received 2007 August 22
- Accepted 2007 October 29
Abstract
In 1997 February, the Japanese radio astronomy satellite HALCA was launched to provide the space-bourne element for the VLBI Space Observatory Program (VSOP) mission. Approximately 25% of the mission time was dedicated to the VSOP survey of bright compact active galactic nuclei (AGNs) at 5 GHz. This paper, the fifth in the series, presents images and models for the remaining 140 sources not included in the third paper in the series, which contained 102 sources. For most sources, the plots of the (u,v) coverage, the visibility amplitude versus (u,v) distance, and the high-resolution image are presented. Model fit parameters to the major radio components are determined, and the brightness temperature of the core component for each source is calculated. The brightness temperature distributions for all of the sources in the VSOP AGN survey are discussed.