VS03j Results
Submitted checklist.txt and checklist.tex is also available
  [Summary | AIPS | Difmap ]
Analyst: Shinjii HORIUCHI
Date Prepared: 22-05-2001
 

Summary
 
Observation code : VS03j    AIPS Version : 15OCT99   
Date of Observation : 1997/337    Difmap Version : 2.3c 
Source Name : J2218-0335    vsop_difmap used : Yes 
Calibration Source(s) :          
Ground telescopes : CD, KA, MP, UD  Model Fitted to data : Yes 
Tracking Station(s) : RZ, NZ, TZ, UZ    Image made : Yes 
Correlator : Penticton         

 
Abstract
Space fringes are detected from UZ tacking baseline. Ceduna has problem with no IF2 data. Kashima shows remarkably low amplitude. From the cross points analysis the factor 2.5 was multiplied with Kashima amplitude. However Kashima data was flagged for the imaging because of low signal to noise most of the time.
Model
Flux (Jy)
Radius (mas)
Theta (deg)
Major (mas)
Axial ratio
Phi (deg)
TB (10^12 K)
0.162786 0.0955426 164.067 0.627985 0.180401 -13.0101 0.1117
(*) 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
 
 
 
 
 
MSORT
 
 
 
 
 
INDXR
 
 
 
 
 
FRING Solint=4, APARM(7)=3, DPARM=1,2000,
   500, 0, REFANT=2
 
 
 
FRING Solint=4, APARM(7)=1, DPARM=1,2000,
   200, 0, REFANT=5
 
 
16 
Only Halcal splution was searched 
TACOP
 
 
 
CLCOR ANTENNA=1,2,3,OPCODE='SBDL',CLPARM(1,2)=-700
 
 
apply off-set for CE, KA, MP 
CLCOR ANTENNA=1,2,3,OPCODE='SBDL',CLPARM(1,2)=700,
TIMERANG = 0/09:00:00.00
   to 0/20:00:00.00
 
 
modification 
CLCOR ANTENNA=2,OPCODE='SBDL',CLPARM(1,2)=100
 
 
apply small off-set for KA 
CLCOR ANTENNA=2,OPCODE='SBDL',CLPARM(1,2)=-100,
TIMERANG = 0/09:00:00.00
   to 0/20:00:00.00
 
 
modification 
CLCOR ANTENNA=1,
   OPCODE='SBDL',CLPARM(1,2)=50,
TIMERANG =0/04:00:00.00 to
   0/09:00:00.00
 
 
modification --------------------------------------------------------- 
CLCOR ANTENNA=4, OPCODE='SBDL',
    CLPARM(1,2)=-730
 
 
apply off-set for again for Halca 
FRING Solint=8, APARM(7)=1, DPARM=1,
   100, 30, 0, REFANT=5
 
 
22 
with narrow search window 
ANTAB
 
 
 
 
TY1, GC1 are generated. 
APCAL
 
 
 
23 
 
CLCAL
23 
 
 
TACOP
 
22 
 
24 
 
SNCOR OPCODE='CLPD',
   SNCORPPRM(1,2)=**
 
24 
 
24 
Clip the bad points for each antena 
CLCAL SMOTYPE = 'VLBI'
24 
 
 
SPLIT
 
 
 
 
FITTP
 
 
 
 
 

AIPS Input Files
Comments
- None -

AIPS Output Files
PRTAN.LIS
LISTR.LIS
DTSUM_0.LIS
DTSUM_1.LIS
POSSM01_AP_02.PS
POSSM01_AP_01.PS
UVPLT_UV.PS
UVPLT_UVD.PS
UVPLT_UVPA.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_FRING2_DEL_1.PS
SN_FRING2_DEL_2.PS
SN_FRING2_RAT_1.PS
SN_FRING2_RAT_2.PS
SN_FRING2_SNR_1.PS
SN_FRING2_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
IMAGE.FITS



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

Image
Ampl, Phase vs (u,v) Distance
PS (40 kb)
JPEG (42 kb)
Ampl, Phase vs Time
PS (213 kb)
JPEG 1, 2, 3
(u,v) Coverage
PS (22 kb)
JPEG (27 kb)
Closure Phase vs Time
PS (244 kb)
JPEG 1, 2
Clean Image
PS (31 kb)
JPEG (73 kb)
Modelfit
Ampl, Phase vs (u,v) Distance
PS (40 kb)
JPEG (41 kb)
Ampl, Phase vs Time
PS (212 kb)
JPEG 1, 2, 3
(u,v) Coverage
PS (22 kb)
JPEG (27 kb)
Closure Phase vs Time
PS (244 kb)
JPEG 1, 2
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)
0.162786 0.0955426 164.067 0.627985 0.180401 -13.0101 0.1117
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



Last updated on Wed May 23 10:46:01 GMT 2001
by db_results.pl version 0.3.