VS09x Results
Submitted checklist.txt and checklist.tex is also available
  [Summary | AIPS | Difmap ]
Analyst: William Scott
Date Prepared: 10-09-2001
 

Summary
 
Observation code : VS09x    AIPS Version : 31DEC00   
Date of Observation : 2000/68    Difmap Version : 2.3c 
Source Name : J1147-07    vsop_difmap used : Yes 
Calibration Source(s) : 1253-055         
Ground telescopes : Mp, Ho, Ka  Model Fitted to data : Yes 
Tracking Station(s) : TZ, GZ    Image made : Yes 
Correlator : Penticton         

 
Abstract
Antenna gain corection factors were accomplished using scalant in DIFMAP, not CLCOR in AIPS. Hence, the FITS file does not have these corrections applied.
Model
Flux (Jy)
Radius (mas)
Theta (deg)
Major (mas)
Axial ratio
Phi (deg)
TB (10^12 K)
0.615357 0.0424901 3.24154 0.556100 0.526928 19.8925 0.1843
(*) 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 DIGICOR=DELCOR=-1
 
 
 
 
Output file name = VS09X.FITLD 
MSORT
 
 
 
 
Input file name = VS09X.FITLD, Output file name = VS09X.UVSRT 
FIXWT
 
 
 
 
Not done. 
INDXR CPARM(1)=3
CPARM(2)=60
CPARM(3)=0.25
 
 
 
 
Created NX(1) 
ANTAB
 
 
 
 
For Ho had Tsys values, and estimated the DPFU. For Ka, Mp, used nominal values. For Halca, used a Tsys of 88K, 92K. 
APCAL
 
 
 
Input: Ty(1) + GC(1) 
CLCAL OPCODE = CALP
INTERPOL = 'AMBG'
REFANT 4 (Mp)
 
 
TBOUT INEXT = 'AN'
 
 
 
 
 
TBIN
 
 
 
 
Changed MNTSTA entries in the AN table. Changed Halca from 3 to 2, and changed Ho to 0. 
TBIN
 
 
 
Read in DQA1 delay and rate solutions. 
SNEDT
 
 
Extremely minor editting of a few discrepant DQA1 solutions. 
CLCAL OPCODE = CALP
INTERPOL = 'AMBG'
REFANT 4 (Mp)
 
 
FRING DOCALIB 1
GAINUSE 3
TIMER 0
SOLINT 4
REFANT 4
SEARCH 2,3
APARM(1)=2
APARM(7)=1 (SNR=1)
DPARM(1)=3 (include baseline
   stacking)
DPARM(2)=50 (50 ns delay
   window)
DPARM(3)=10 (10mHz rate
   window)
DPARM(4)=0.5
DPARM(5)=0
DPARM(6)=1
 
 
Solutions looked great. 
SNEDT
 
 
Minor editting. 
CLCAL OPCODE='CALP'
INTERPOL = 'AMBG'
SMOTYPE = ''
REFANT 8
 
 
SPLIT SOURCES 'J1147-07'
DOCALIB 1, GAINUSE 4
 
 
 
Input file: VS09X.UVSRT, Output file: J1147-07.FITS, 1253-055.FITS 
FITTP
 
 
 
 
Input file: J1147-07.FITS, 1253-055.FITS Output file: J1147-07.FITS, 1253-055.FITS amplitude 

AIPS Input Files
ANTAB.TXT
INDXR.TXT
Comments
- None -

AIPS Output Files
DTSUM_0.LIS
DTSUM_1.LIS
LISTR.LIS
PRTAN.LIS
POSSM01_AP_1.PS
POSSM02_AP_1.PS
SN_APCAL_AMP_1.PS
SN_APCAL_AMP_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
UVPLT_UV.PS
UVPLT_UVD.PS
UVPLT_UVPA.PS
VPLOT_AP_1.PS
VPLOT_AP_2.PS
WEIGHTS.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
Applied a root(2) correction factor to all the antennas with scalant (NOT CLCOR in AIPS). Also, corrected Ho and Ka by factors of 1.2 and 2.8 respectively (again with scalant). Used crossing points to determine these scaling factors. Did not use gscale. Final image had a slight extension to the west, consistent with the PLS. Used UVTAPER to pick up the extended emission. When correction factor were applied the zerospacing visibilities for the fringe finder (3C279) was consistent with the AT light curve zerospacing flux.

Image
Ampl, Phase vs (u,v) Distance
PS (81 kb)
JPEG (51 kb)
Ampl, Phase vs Time
PS (186 kb)
JPEG 1, 2
(u,v) Coverage
PS (40 kb)
JPEG (31 kb)
Closure Phase vs Time
PS (125 kb)
JPEG 1
Clean Image
PS (37 kb)
JPEG (47 kb)
Modelfit
Ampl, Phase vs (u,v) Distance
PS (81 kb)
JPEG (51 kb)
Ampl, Phase vs Time
PS (185 kb)
JPEG 1, 2
(u,v) Coverage
PS (40 kb)
JPEG (31 kb)
Closure Phase vs Time
PS (123 kb)
JPEG 1
Image with model components
PS (38 kb)
JPEG (40 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)
0.615357 0.0424901 3.24154 0.556100 0.526928 19.8925 0.1843
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



Last updated on Wed Aug 25 07:24:52 GMT 2004
by db_results.pl version 0.3.