VS06u Results
Submitted checklist.txt and checklist.tex is also available
  [Summary | AIPS | Difmap ]
Analyst: Shinjii HORIUCHI
Date Prepared: 21-05-2001
 

Summary
 
Observation code : VS06u    AIPS Version : 15OCT99   
Date of Observation : 1999/145    Difmap Version : 2.3c 
Source Name : J1257-3155    vsop_difmap used : Yes 
Calibration Source(s) : 1255-316         
Ground telescopes : HO, SH, HA  Model Fitted to data : Yes 
Tracking Station(s) : UZ, RZ    Image made : Yes 
Correlator : Penticton         

 
Abstract
Data was correlated in non-standard mode with 64 channels. Space fringes are detected from RZ. The UZ might have problem. Due to unkown reason all baselines show remakably low amplitude and hence, derived factors are multiplied in AIPS.
Model
Flux (Jy)
Radius (mas)
Theta (deg)
Major (mas)
Axial ratio
Phi (deg)
TB (10^12 K)
1.58352 0.00468734 -9.03668 0.369249 0.859140 10.7333 0.6597
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



AIPS Data Reduction Notes
 
Task
Adverbs
CL
in
SN
in
CL
out
SN
out
Comments
FITLD
 
 
 
 
 
INDXR
 
 
 
 
 
ACCOR SOLINT=10
 
 
 
 
CLCAL SMOTYPE = 'AMPL'
 
FRING SOLINT=20, REFANT=1,
   DOFIT=4,5
APARM(7)=0.1, DPARM=1,600, 20, 0 
 
 
Space only solution 
FRING SOLINT=20, REFANT=1,
   DOFIT=DOFIT1,2,3
APARM(7)=0.1, DPARM=1,110, 20, 0 
 
 
Ground only solution 
CLCAL SMOTYPE = 'VLBI'
 
 
CLCAL SMOTYPE = 'VLBI'
 
 
ANTAB
 
 
 
 
TY1, GC1 are generated. 
APCAL
 
 
 
 
CLCAL SMOTYPE = 'AMPL'
 
 
TACOP
 
 
 
CLCOR OPCODE = 'GAIN', ANTENNAS
    = 1, CLPARM = 1.20000E+00,
   0
 
 
 
CLCOR OPCODE = 'GAIN', ANTENNAS
    = 2, CLPARM = 2.50000E+00,
   0
 
 
 
CLCOR OPCODE = 'GAIN',A NTENNAS
    = 3, CLPARM = 3.80000E+00,
   0
 
 
 
SPLIT
 
 
 
 
FITTP
 
 
 
 
 

AIPS Input Files
Comments
- None -

AIPS Output Files
PRTAN.LIS
LISTR.LIS
DTSUM_0.LIS
DTSUM_1.LIS
POSSM01_AP_01.PS
POSSM01_AP_02.PS
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_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_FRING05_DEL_1.PS
SN_FRING05_DEL_2.PS
SN_FRING05_RAT_1.PS
SN_FRING05_RAT_2.PS
SN_FRING05_SNR_1.PS
SN_FRING05_SNR_2.PS
SN_FRING06_DEL_1.PS
SN_FRING06_DEL_2.PS
SN_FRING06_RAT_1.PS
SN_FRING06_RAT_2.PS
SN_FRING06_SNR_1.PS
SN_FRING06_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



Difmap Data Reduction Notes
Phase selfcal applied? Yes
Global amplitude selfcal (gscal) applied? Yes
Amplitude selfcal on non-global timescales used? Yes
Modelfit made and saved? Yes
Image Made and saved? Yes
Comments on Difmap processing
The global amp. selfcal and short time interval amp. selfcal were applied. The source may consists of two compact cores components.

Image
Ampl, Phase vs (u,v) Distance
PS (53 kb)
JPEG (49 kb)
Ampl, Phase vs Time
PS (143 kb)
JPEG 1, 2
(u,v) Coverage
PS (28 kb)
JPEG (31 kb)
Closure Phase vs Time
PS (99 kb)
JPEG 1
Clean Image
PS (41 kb)
JPEG (47 kb)
Modelfit
Ampl, Phase vs (u,v) Distance
PS (53 kb)
JPEG (49 kb)
Ampl, Phase vs Time
PS (143 kb)
JPEG 1, 2
(u,v) Coverage
PS (28 kb)
JPEG (31 kb)
Closure Phase vs Time
PS (99 kb)
JPEG 1
Image with model components
PS (31 kb)
JPEG (37 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)
1.58352 0.00468734 -9.03668 0.369249 0.859140 10.7333 0.6597
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



Last updated on Wed May 23 01:54:51 GMT 2001
by db_results.pl version 0.3.