VSOP Survey Program observation of J2232+1143

J2232+1143

The data on this page are described in detail in
The VSOP 5 GHz AGN Survey: V. Imaging results for the remaining 140 sources
by Dodson et al. in Astrophysical Journal Supplement, 175, 314-355 (May 2008) .
Please refer to this paper for details of the observations, analysis and interpretation.

The observation of J2232+1143 (2230+114CTA102) was made on 1998-May-25
with HALCA and 4 ground radio-telescopes over a duration of 04:00 (hours:minutes).
Baselines to HALCA were not necessarily available for all of that time.
The survey code for this source is vs01w*.
The observation was correlated at the Socorro correlator.
The source is classified as a object at a redshift of 1.037.
Please refer to the paper for full details and references.

Results from modelfitting Gaussian components to the data

  
                                 major   minor          Brightness  
Source        S      r     PA    axis    axis     PA    Temperature 
name         (Jy)  (mas)  (deg)  (mas)   (mas)   (deg)  (10^12 K) 

J2232+1143     1.44   0.1   137   0.4   0.4   ...      0.61 
               0.87   1.8   140   0.5   0.5   ...     
               1.14   7.6   159   2.1   2.1   ...     
               0.82   5.8   145   1.9   1.9   ...     
               0.91   25.5   143   3.7   3.7   ...

Specific notes in the above paper for this source are:

VSOP Survey Program image at 5 GHz
contour png | contour ps.gz

Correlated flux density (Jy) vs. projected baseline length plot
png | ps.gz

(u,v) coverage for the observation
png | ps.gz

Last modified: 2008-08-16