vs07a Results
Submitted checklist.txt and checklist.tex is also available
  [Summary | AIPS | Difmap ]
Analyst: Glenn Piner
Date Prepared: 16-06-1999
 

Summary
 
Observation code : vs07a    AIPS Version : 15APR99   
Date of Observation : 1998/61    Difmap Version : 2.3c 
Source Name : 0016+731    vsop_difmap used : Yes 
Calibration Source(s) :          
Ground telescopes : LA,MK,SC  Model Fitted to data : Yes 
Tracking Station(s) : GZ,NZ    Image made : Yes 
Correlator : Socorro         

 
Abstract
These survey products were generated from an already-reduced GOT dataset (V030a). The fully reduced GOT data were used to produce the survey-required AIPS plots (adhering as closely as possible to the most recently released VSOP survey documentation and scripts). A subset of antennas and timeranges were extracted to produce the VSOP survey dataset and the imaging and model-fitting for the survey were done on this "extracted" dataset.

In order to find weak HALCA fringes, the ground telescopes were fringed first. These solutions were applied and the resulting data was averaged in frequency and time using SPLAT. This helped increase the SNR for the weak HALCA fringes. Because of this, the GRTs in the final fringe plots have zero delays and rates, and there are two TASAV files: the final version and the tables as they were before SPLAT was applied.

Suggested parameters for all AIPS tasks were used. CALIB was not run so the final SN and CL tables have non-zero phases in them. This dataset came from Steven Tingay and Matt Lister.

Model
Flux (Jy)
Radius (mas)
Theta (deg)
Major (mas)
Axial ratio
Phi (deg)
TB (10^12 K)
0.255075 0.163932 -88.2381 0.762842 0.632741 -18.6462 0.0338
0.121334 0.358130 102.288 0.241498 0.751295 -55.9231 0.1351
0.0302541 0.852236 132.487 0 0 0 0.0000
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



AIPS Data Reduction Notes
 
- None -

AIPS Input Files
UVFLG.TXT
ANTAB.TXT
Comments
- None -

AIPS Output Files
DTSUM_0.LIS
DTSUM_1.LIS
PRTAN.LIS
LISTR.LIS
SN_CALIB_SNR_1.PS
UVPLT_UV.PS
POSSM01_AP_1.PS
UVPLT_UVD.PS
UVPLT_UVPA.PS
SN_ACCOR_AMP_1.PS
SN_ACCOR_AMP_2.PS
SN_APCAL_AMP_1.PS
SN_APCAL_AMP_2.PS
SN_CALIB_DEL_1.PS
SN_CALIB_DEL_2.PS
SN_CALIB_PHA_1.PS
SN_CALIB_PHA_2.PS
SN_CALIB_RAT_1.PS
SN_CALIB_RAT_2.PS
VPLOT_AP_1.PS
VPLOT_AP_2.PS
SN_CALIB_SNR_2.PS
POSSM01_AP_2.PS
POSSM02_AP_2.Ps
POSSM02_AP_1.PS



Difmap Data Reduction Notes
Phase selfcal applied? No
Global amplitude selfcal (gscal) applied? No
Amplitude selfcal on non-global timescales used? No
Modelfit made and saved? Yes
Image Made and saved? Yes
Comments on Difmap processing

Image
Ampl, Phase vs (u,v) Distance
PS (71 kb)
GIF (8 kb)
Ampl, Phase vs Time
PS (2257 kb)
GIF 1, 2, 3, 4, 5, 6, 7
(u,v) Coverage
PS (34 kb)
GIF (5 kb)
Closure Phase vs Time
PS (6667 kb)
GIF 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 23, 24, 25, 26, 27
Clean Image
PS (33 kb)
GIF (55 kb)
Modelfit
Ampl, Phase vs (u,v) Distance
PS (71 kb)
GIF (8 kb)
Ampl, Phase vs Time
PS (2255 kb)
GIF 1, 2, 3, 4, 5, 6, 7
(u,v) Coverage
PS (34 kb)
GIF (5 kb)
Closure Phase vs Time
PS (6668 kb)
GIF 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 23, 24, 25, 26, 27
Image with model components
PS (33 kb)
GIF (7 kb)

More details on the Images and Modelfits are found in this page.

Model
Flux (Jy)
Radius (mas)
Theta (deg)
Major (mas)
Axial ratio
Phi (deg)
TB (10^12 K)
0.255075 0.163932 -88.2381 0.762842 0.632741 -18.6462 0.0338
0.121334 0.358130 102.288 0.241498 0.751295 -55.9231 0.1351
0.0302541 0.852236 132.487 0 0 0 0.0000
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



Last updated on Mon Nov 22 08:31:33 GMT 1999
by db_results.pl version 0.2.0.