vs01g Results
Submitted checklist.txt and checklist.tex is also available
  [Summary | AIPS | Difmap ]
Analyst: Glenn Piner
Date Prepared: 17-06-1999
 

Summary
 
Observation code : vs01g    AIPS Version : 15APR99   
Date of Observation : 1998/10    Difmap Version : 2.3c 
Source Name : 3C279    vsop_difmap used : Yes 
Calibration Source(s) : 1213-172 1334-127         
Ground telescopes : KP,MK,SC  Model Fitted to data : Yes 
Tracking Station(s) : RZ    Image made : Yes 
Correlator : Socorro         

 
Abstract
These survey products were generated from an already-reduced GOT dataset (V147b1). 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.

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.

Imaging and model-fitting both went very well and produced good results.

Model
Flux (Jy)
Radius (mas)
Theta (deg)
Major (mas)
Axial ratio
Phi (deg)
TB (10^12 K)
3.58271 0.0417786 116.622 0.177398 0.467172 74.1486 11.8921
2.93587 0.356388 -127.967 0.163243 1.00000 0.00000 5.3763
0.409584 1.13130 -134.569 0.157316 1.00000 11.3099 0.8076
5.33668 3.15752 -112.704 1.51378 0.246704 16.1119 0.4607
(*) 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_1.LIS
PRTAN.LIS
LISTR.LIS
DTSUM_0.LIS
UVPLT_UV.PS
SN_CALIB_DEL_2.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_PHA_1.PS
SN_CALIB_PHA_2.PS
SN_CALIB_RAT_1.PS
SN_CALIB_RAT_2.PS
SN_CALIB_SNR_1.PS
SN_CALIB_SNR_2.PS
VPLOT_AP_1.PS
VPLOT_AP_2.PS
POSSM01_AP_2.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 (39 kb)
GIF (7 kb)
Ampl, Phase vs Time
PS (1451 kb)
GIF 1, 2, 3, 4, 5, 6
(u,v) Coverage
PS (20 kb)
GIF (4 kb)
Closure Phase vs Time
PS (3631 kb)
GIF 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16
Clean Image
PS (44 kb)
GIF (53 kb)
Modelfit
Ampl, Phase vs (u,v) Distance
PS (39 kb)
GIF (7 kb)
Ampl, Phase vs Time
PS (1451 kb)
GIF 1, 2, 3, 4, 5, 6
(u,v) Coverage
PS (20 kb)
GIF (4 kb)
Closure Phase vs Time
PS (3631 kb)
GIF 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16
Image with model components
PS (44 kb)
GIF (9 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)
3.58271 0.0417786 116.622 0.177398 0.467172 74.1486 11.8921
2.93587 0.356388 -127.967 0.163243 1.00000 0.00000 5.3763
0.409584 1.13130 -134.569 0.157316 1.00000 11.3099 0.8076
5.33668 3.15752 -112.704 1.51378 0.246704 16.1119 0.4607
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



Last updated on Mon Nov 22 07:52:08 GMT 1999
by db_results.pl version 0.2.0.