vs03o Results
Submitted checklist.txt and checklist.tex is also available
  [Summary | AIPS | Difmap ]
Analyst: Glenn Piner
Date Prepared: 18-06-1999
 

Summary
 
Observation code : vs03o    AIPS Version : 15APR99   
Date of Observation : 1998/181    Difmap Version : 2.3c 
Source Name : 1404+286    vsop_difmap used : Yes 
Calibration Source(s) :          
Ground telescopes : EB,HN,SC  Model Fitted to data : Yes 
Tracking Station(s) : TZ    Image made : Yes 
Correlator : Socorro         

 
Abstract
This survey dataset is an extraction of the GOT experiment v085q. The extraction was received on tape from Socorro containing data from the EB, HN, NL, and SC GRTs plus HALCA, over a 3 hour time range. The NL data was flagged before imaging in Difmap.

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. 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.

Imaging this source was difficult with only 3 GRTs. Fringes were found to HALCA over only ~1/2 of the 3 hour time range. While an image with all 4 GRTs recovers the source structure, flagging any of the remaining GRTs significantly worsens the image.

Model
Flux (Jy)
Radius (mas)
Theta (deg)
Major (mas)
Axial ratio
Phi (deg)
TB (10^12 K)
1.12331 0.0281592 11.1529 0.763428 0.523847 -19.7416 0.1795
0.0531209 0.308445 -127.979 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
PRTAN.LIS
LISTR.LIS
DTSUM_0.LIS
DTSUM_1.LIS
UVPLT_UV.PS
UVPLT_UVD.PS
UVPLT_UVPA.PS
SN_ACCOR_AMP_1.PS
SN_ACCOR_AMP_2.PS
SN_APCAL_AMP_2.PS
SN_APCAL_AMP_1.PS
SN_FRING01_DEL_1.PS
SN_FRING01_DEL_2.PS
SN_FRING01_RAT_1.PS
SN_FRING01_RAT_2.PS
SN_FRING01_SNR_1.PS
SN_FRING01_SNR_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
SN_CALIB_SNR_1.PS
SN_CALIB_SNR_2.PS
SN_FRING02_DEL_1.PS
SN_FRING02_DEL_2.PS
SN_FRING02_RAT_1.PS
SN_FRING02_RAT_2.PS
SN_FRING02_SNR_1.PS
SN_FRING02_SNR_2.PS
VPLOT_AP_1.PS
VPLOT_AP_2.PS
POSSM01_AP_1.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 (27 kb)
GIF (6 kb)
Ampl, Phase vs Time
PS (200 kb)
GIF 1, 2, 3
(u,v) Coverage
PS (16 kb)
GIF (4 kb)
Closure Phase vs Time
PS (239 kb)
GIF 1, 2
Clean Image
PS (38 kb)
GIF (62 kb)
Modelfit
Ampl, Phase vs (u,v) Distance
PS (27 kb)
GIF (6 kb)
Ampl, Phase vs Time
PS (202 kb)
GIF 1, 2, 3
(u,v) Coverage
PS (16 kb)
GIF (4 kb)
Closure Phase vs Time
PS (237 kb)
GIF 1, 2
Image with model components
PS (37 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)
1.12331 0.0281592 11.1529 0.763428 0.523847 -19.7416 0.1795
0.0531209 0.308445 -127.979 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 08:19:10 GMT 1999
by db_results.pl version 0.2.0.