VS05n Results
Submitted checklist.txt and checklist.tex is also available
  [Summary | AIPS | Difmap ]
Analyst: William Scott
Date Prepared: 28-08-2002
 

Summary
 
Observation code : VS05n    AIPS Version : 31Dec00   
Date of Observation : 2002/58    Difmap Version : 2.3c 
Source Name : J0457-23    vsop_difmap used : Yes 
Calibration Source(s) : J0609-15         
Ground telescopes : Ka, Ho, Mp  Model Fitted to data : Yes 
Tracking Station(s) : UZ    Image made : Yes 
Correlator : Penticton         

 
Abstract
Model
Flux (Jy)
Radius (mas)
Theta (deg)
Major (mas)
Axial ratio
Phi (deg)
TB (10^12 K)
1.80952 0.0615357 -40.0691 0 0 0 0.0000
2.13146 0.315962 -115.619 0.739081 1.00000 -31.0106 0.1904
(*) 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 = VS05N.FITLD 
MSORT
 
 
 
 
Input file name = VS05N.FITLD, Output file name = VS05N.UVSRT 
FIXWT
 
 
 
 
Not done. 
INDXR CPARM(1)=3
CPARM(2)=60
CPARM(3)=0.25
 
 
 
 
No CSEs. Created NX(1) 
ANTAB
 
 
 
 
For Halca used a Tsys of 88K, 92K. For Mp used a nominal SEFD of 450 Jy. For Ka used a nominal Tsys of 171K, and a nominal DPFU of 0.26. For Ho, had Tsys vals around 170 (K). Assumed these are actually SEFDs/10 (although this is a little higher than what I would normally expect). 
APCAL
 
 
 
Input: Ty(1) + GC(1) 
CLCAL OPCODE = CALP
INTERPOL = 'AMBG'
REFANT 3 (Mp)
 
Used Mp as refant. 
TBOUT INEXT = 'AN'
 
 
 
 
 
TBIN
 
 
 
 
Changed MNTSTA entries in the AN table. Changed Halca from 3 to 2, and changed Ho from 2 to 0. 
TBIN
 
 
 
Read in DQA1 delay and rate solutions using antenna 5 (Mp) as the reference antenna. 
SNEDT
 
 
Minor editting of DQA1 rate solutions. 
CLCAL OPCODE = CALP
INTERPOL = 'AMBG'
REFANT 3
 
 
FRING DOCALIB 1
GAINUSE 3
TIMER 0
SOLINT 2
REFANT 3 (Mp)
SEARCH 2,3
APARM(1)=2
APARM(7)=3 (SNR=3)
DPARM(1)=3 (include baseline
   stacking)
DPARM(2)=20 (20 ns delay
   window)
DPARM(3)=40 (40mHz rate
   window)
DPARM(4)=0.5
DPARM(5)=0
DPARM(6)=1
 
 
Used a smallish SOLINT and largish DPARM(3) since the rates for Halca in the DQA1 report were fairly high. 
SNEDT
 
 
Minor editting. 
CLCAL OPCODE='CALP'
INTERPOL = 'AMBG'
SMOTYPE = ''
REFANT 3
 
 
CLCOR
 
 
 
 
Since this experiment was correlated on Jun 05/02, no corrections for the correlator need be applied. 
SPLIT SOURCES 'J0457-23','J0609-15'
DOCALIB 1, GAINUSE 4
 
 
 
Input file: VS05N.UVSRT, Output file: J0609-15.VS05N,J0457-23.VS05N 
FITTP
 
 
 
 
Input files: J0609-15.VS05N,J0457-23.VS05N Output files: J0609-15.FITS,J0457-23.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
UVPLT_UV.PS
SN_CALIB_SNR_1.PS
SN_CALIB_SNR_2.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? No
Amplitude selfcal on non-global timescales used? No
Modelfit made and saved? Yes
Image Made and saved? Yes
Comments on Difmap processing
Did not use gscale. Used a uv-taper to pick up some more diffuse emission.

Image
Ampl, Phase vs (u,v) Distance
PS (44 kb)
JPEG (38 kb)
Ampl, Phase vs Time
PS (130 kb)
JPEG 1, 2
(u,v) Coverage
PS (23 kb)
JPEG (27 kb)
Closure Phase vs Time
PS (98 kb)
JPEG 1
Clean Image
PS (37 kb)
JPEG (44 kb)
Modelfit
Ampl, Phase vs (u,v) Distance
PS (44 kb)
JPEG (38 kb)
Ampl, Phase vs Time
PS (130 kb)
JPEG 1, 2
(u,v) Coverage
PS (23 kb)
JPEG (27 kb)
Closure Phase vs Time
PS (97 kb)
JPEG 1
Image with model components
PS (43 kb)
JPEG (42 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)
1.80952 0.0615357 -40.0691 0 0 0 0.0000
2.13146 0.315962 -115.619 0.739081 1.00000 -31.0106 0.1904
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



Last updated on Wed Aug 25 07:05:47 GMT 2004
by db_results.pl version 0.3.