VS06k Results
Submitted checklist.txt and checklist.tex is also available
  [Summary | AIPS | Difmap ]
Analyst: William Scott
Date Prepared: 15-11-2001
 

Summary
 
Observation code : VS06k    AIPS Version : 31Dec01   
Date of Observation : 2000/345    Difmap Version : 2.3c 
Source Name : J2358-10    vsop_difmap used : Yes 
Calibration Source(s) : J0050-09         
Ground telescopes : Mp, AT, Hh  Model Fitted to data : Yes 
Tracking Station(s) : RZ    Image made : Yes 
Correlator : Penticton         

 
Abstract
Data extraction from experiment W001e. AT light curves gave a zero spacing flux of about 0.6 Jy around December 1999 (about a year before this observation). Source was highly variable...3 years earlier it had a zero spacing flux of about 1.6 Jy.
Model
Flux (Jy)
Radius (mas)
Theta (deg)
Major (mas)
Axial ratio
Phi (deg)
TB (10^12 K)
1.70699 0.112733 21.2299 3.10522 0.104843 -3.49746 0.0824
(*) 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 = VS06K.FITLD 
MSORT
 
 
 
 
Input file name = VS06K.FITLD, Output file name = VS06K.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. Used nominal Tsys and DPFU values for the AT and Mp. As far as I could tell all 6 antennas in the AT participated in the experiment. Hh had Tsys values supplied. 
APCAL
 
 
 
Input: Ty(1) + GC(1) 
UVFLG OPCODE = REAS
REASON 'NO PRC/LOW DVAL'
 
 
 
 
Needed to unflag the NO PRC/LOW DVAL data... as per the piletter most of this data was ok. 
CLCAL OPCODE = CALP
INTERPOL = '2PT'
REFANT 4 (Mp)
 
Used Mp as refant for now, since it had the most "good" solutions in the Penticton DQA1 report. 
TBOUT INEXT = 'AN'
 
 
 
 
 
TBIN
 
 
 
 
Changed MNTSTA entries in the AN table. Changed Halca from 3 to 2, and changed all other antennas to 0. 
TBIN
 
 
 
Read in DQA1 delay and rate solutions using antenna 4 (Mp) as the reference antenna. antenna. Note: had to do lots of modifications to the SN table before it was read in, since there were many cases where there were good solutions for one IF, but not for the other. This caused CLCAL to do unpredicable things when it interpolated. 
SNEDT
 
 
Minor editting of DQA1 solutions. 
CLCAL OPCODE = CALP
INTERPOL = 'AMBG'
REFANT 4 (Mp)
 
 
UVFLG OPCODE = REAS
REASON = 'NO PRC/LOW DVAL'
 
 
 
 
Need to unedit some of the NO PRC/LOW DVAL flags before running FRING, since otherwise half of the Mp data is flagged out. 
FRING DOCALIB 1
GAINUSE 3
TIMER 0
SOLINT 2
REFANT 1 (AT)
SEARCH 4,2
APARM(1)=2
APARM(7)=3 (SNR=3)
DPARM(1)=3 (include baseline
   stacking)
DPARM(2)=30 (30 ns delay
   window)
DPARM(3)=20 (20mHz rate
   window)
DPARM(4)=0.5
DPARM(5)=0
DPARM(6)=1
 
 
 
SNEDT
 
 
Minor editting of DQA1 solutions. 
CLCAL OPCODE = CALP
INTERPOL = 'AMBG'
REFANT 1 (AT)
 
 
FRING DOCALIB 1
GAINUSE 3
TIMER 0 0 0 0 0 11 44 52
SOLINT 5
REFANT 1 (AT)
SEARCH 4,2
APARM(1)=2
APARM(7)=3 (SNR=3)
DPARM(1)=3 (include baseline
   stacking)
DPARM(2)=30 (30 ns delay
   window)
DPARM(3)=20 (20mHz rate
   window)
DPARM(4)=0.5
DPARM(5)=0
DPARM(6)=1
 
 
 
SNEDT
 
 
Minor editting of DQA1 solutions. 
CLCAL OPCODE = CALP
INTERPOL = 'AMBG'
REFANT 1 (AT)
 
 
TACOP
 
 
 
CLCOR OPCODE 'GAIN'
ANTENNAS 0
CLCORPRM 1.19,0
 
 
Lots of problems to determine gain corrections. Data for calibrator J2148+06 was out by a factor of 10, and was inconsistent with the other data... did not use to determine the gain correction factors. No AT or UMRAO single dish observations of the source around the obs time. Small spacing flux for calibrator J0050-09 lower than PLS flux by about a factor of 7.5. For J0050-06 Hh-AT and Hh-Mp baselines should have almost been identical, but were out by about a factor of 4 and 8 for IFs 1 and 2. Made the assumption J0050-06 was still unresolved as it was in the PLS, and with the PLS flux of 1.5Jy. Added the the sqrt(2) gain factor then made successive CLCOR corrections to further modify the antenna gains. 
CLCOR OPCODE 'GAIN'
ANTENNAS 1 (AT)
CLCORPRM 4.7 for IF1, and
   8.1 for IF2
 
 
 
CLCOR OPCODE 'GAIN'
ANTENNAS 2 (Hh)
CLCORPRM 2.3 for IF1, and
   2.6 for IF2
 
 
 
CLCOR OPCODE 'GAIN'
ANTENNAS 4 (Mp)
CLCORPRM 1.2 for IF1
 
 
 
SPLIT SOURCES 'J2358-10'
DOCALIB 1, GAINUSE 6
 
 
 
Input file: VS06K.UVSRT, Output file: J2358-10.FITS Looked at DIFMAP solutions in three cases, with only DQA1 TBIN solutions, with DQA1 solutions but then fringed with solint=2, and with DQA1 solutions but then fringed with solint=5. Second case was the worst (fewer solutions were found). Had marginally better luck without fringing with solint=5, so split with the CL table that had no fringing done (ie: CL(3), which was copied to CL(6)). 
FITTP
 
 
 
 
Input file: J2358-10.FITS Output file: J2358-10.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
POSSM03_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
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
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? No
Amplitude selfcal on non-global timescales used? No
Modelfit made and saved? Yes
Image Made and saved? Yes
Comments on Difmap processing
No gscale applied. Had to play with uvtaper a lot in order to get sufficient flux on the short baselines.

Image
Ampl, Phase vs (u,v) Distance
PS (47 kb)
JPEG (43 kb)
Ampl, Phase vs Time
PS (150 kb)
JPEG 1, 2
(u,v) Coverage
PS (26 kb)
JPEG (26 kb)
Closure Phase vs Time
PS (110 kb)
JPEG 1
Clean Image
PS (39 kb)
JPEG (46 kb)
Modelfit
Ampl, Phase vs (u,v) Distance
PS (47 kb)
JPEG (44 kb)
Ampl, Phase vs Time
PS (149 kb)
JPEG 1, 2
(u,v) Coverage
PS (26 kb)
JPEG (26 kb)
Closure Phase vs Time
PS (109 kb)
JPEG 1
Image with model components
PS (44 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)
1.70699 0.112733 21.2299 3.10522 0.104843 -3.49746 0.0824
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



Last updated on Wed Aug 25 07:26:05 GMT 2004
by db_results.pl version 0.3.