VS11f Results
Submitted checklist.txt and checklist.tex is also available
  [Summary | AIPS | Difmap ]
Analyst: Zhi-Qiang Shen
Date Prepared: 05-07-1999
 

Summary
 
Observation code : VS11f    AIPS Version : 15OCT98   
Date of Observation : 1998/52    Difmap Version : 2.3c 
Source Name : J1035-20    vsop_difmap used : Yes 
Calibration Source(s) : 1253-055         
Ground telescopes : HartRAO, Mop, Hobart, Usuda64  Model Fitted to data : Yes 
Tracking Station(s) : GZ    Image made : Yes 
Correlator : Penticton         

 
Abstract
Strong fringes were detected on most ground-ground baselines except those to Mop and Hobart. Mop also had problem with amplitude gains which can be seen from both survey source and calibration source data. Hobart gains were multiplied by a factor of ~0.6 to match the adopted DPFU of 0.1 and the measured Tsys of ~300K.

For ground-space baselines, good fringes were detected during the entire GZ pass (14:58 -- 18:16 UT).

Imaging with DIFMAP showed a compact central component with some possible emission to the south. To keep simple, a circular Gaussian component model was adopted to fit the calibrated data of the survey source J1658+07.

The calibrator 1253-055 has a correlated flux density of 5.1 Jy on the baseline HARTRAO-HOBART of 9,000 km.

Model
Flux (Jy)
Radius (mas)
Theta (deg)
Major (mas)
Axial ratio
Phi (deg)
TB (10^12 K)
0.249667 0.00000 0.00000 0.0916571 1.00000 0.00000 1.4503
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



AIPS Data Reduction Notes
 
- None -

AIPS Input Files
INDXR.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_APCAL_AMP_1.PS
SN_APCAL_AMP_2.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_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
SN_FRING03_DEL_1.PS
SN_FRING03_DEL_2.PS
SN_FRING03_RAT_1.PS
SN_FRING03_RAT_2.PS
SN_FRING03_SNR_1.PS
SN_FRING03_SNR_2.PS
SN_FRING04_DEL_1.PS
SN_FRING04_DEL_2.PS
SN_FRING04_RAT_1.PS
SN_FRING04_RAT_2.PS
SN_FRING04_SNR_1.PS
SN_FRING04_SNR_2.PS
SN_CALIB_DEL_1.PS
SN_CALIB_DEL_2.PS
SN_CALIB_RAT_1.PS
SN_CALIB_RAT_2.PS
SN_CALIB_SNR_1.PS
SN_CALIB_SNR_2.PS
SN_CALIB_PHA_1.PS
SN_CALIB_PHA_2.PS
POSSM01_AP_1.PS
POSSM01_AP_2.PS
VPLOT_AP_1.PS
VPLOT_AP_2.PS
IMAGE.FITS



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 (37 kb)
GIF (6 kb)
Ampl, Phase vs Time
PS (232 kb)
GIF 1, 2, 3
(u,v) Coverage
PS (20 kb)
GIF (4 kb)
Closure Phase vs Time
PS (254 kb)
GIF 1, 2
Clean Image
PS (33 kb)
GIF (81 kb)
Modelfit
Ampl, Phase vs (u,v) Distance
PS (37 kb)
GIF (6 kb)
Ampl, Phase vs Time
PS (232 kb)
GIF 1, 2, 3
(u,v) Coverage
PS (20 kb)
GIF (4 kb)
Closure Phase vs Time
PS (254 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)
0.249667 0.00000 0.00000 0.0916571 1.00000 0.00000 1.4503
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



Last updated on Mon Nov 22 07:44:26 GMT 1999
by db_results.pl version 0.2.0.