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J/ApJS/175/314 VSOP 5GHz AGN survey V. (Dodson+, 2008)
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Beginning of ReadMe :J/ApJS/175/314 VSOP 5GHz AGN survey V. (Dodson+, 2008)
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The VSOP 5 GHz active galactic nucleus survey.
V. Imaging results for the remaining 140 sources.
Dodson R., Fomalont E.B., Wiik K., Horiuchi S., Hirabayashi H.,
Edwards P.G., Murata Y., Asaki Y., Moellenbrock G.A., Scott W.K.,
Taylor A.R., Gurvits L.I., Paragi Z., Frey S., Shen Z.-Q., Lovell J.E.J.,
Tingay S.J., Rioja M.J., Fodor S., Lister M.L., Mosoni L., Coldwell G.,
Piner B.G., Yang J.
<Astrophys. J. Suppl. Ser., 175, 314-355 (2008)>
=2008ApJS..175..314D
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ADC_Keywords: Active gal. nuclei ; Radio continuum ; Surveys
Keywords: galaxies: active - radio continuum: galaxies - surveys
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 5GHz. 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.
Description:
The VSOP mission and the 5GHz AGN Survey are fully discussed in
Hirabayashi et al. (1998Sci...281.1825H, 2000PASJ...52..955H),
Paper I (Hirabayashi et al., 2000, Cat J/PASJ/52/997), and
Fomalont et al. (2000, Cat. J/ApJS/131/95). Observations began in
1997 August, with the final observations being made in 2003 October.
Of the VSS sample of 294 sources, all but 29 were observed.