VS03e Results
Submitted checklist.txt and checklist.tex is also available
  [Summary | AIPS | Difmap ]
Analyst: William Scott
Date Prepared: 05-07-1999
 

Summary
 
Observation code : VS03e    AIPS Version : 15APR99   
Date of Observation : 1998/231    Difmap Version : 2.3c 
Source Name : J0405-13    vsop_difmap used : Yes 
Calibration Source(s) : 0420-014         
Ground telescopes : Sh, Mp  Model Fitted to data : Yes 
Tracking Station(s) : RZ, GZ    Image made : Yes 
Correlator : Penticton         

 
Abstract
Model
Flux (Jy)
Radius (mas)
Theta (deg)
Major (mas)
Axial ratio
Phi (deg)
TB (10^12 K)
0.411363 0.0123678 131.683 0.194289 1.00000 22.6356 0.5318
(*) 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 = VS03E.FITLD 
MSORT
 
 
 
 
Input file name = VS03E.FITLD, Output file name = VS03E.UVSRT 
FIXWT CPARM(1)=3
CPARM(3)=0.25 = Cl table
   time interval
 
 
 
Input file name = VS03E.UVSRT, Output file name = VS03E.FIXWT 
INDXR
 
 
 
 
Created NX(1) 
OBTAB
 
 
 
 
Not Used 
TABPUT
 
 
 
 
Changed entries in AN(1) for MNTSTA, ie: VSOP_SC from 3 to 2, 
UVFLG TIMER 0 18 0 0 0 23 0 0
ANTENNAS 0
BASELINE 0
OPCODE 'REAS'
REASON 'NO PRC/LOW DVA'
 
 
 
 
Unflagged all the data in the second tracking pass that was flagged due to 'NO PRC/LOW DVA'. This was due to a bad transport (cf. the PI letter), so this data should be ok, but with a slightly lower SNR. 
IBLED
 
 
 
 
Edits stored in FG(1). 
ACCOR
 
 
 
 
Not Used 
ANTAB
 
 
 
 
INFILE='CAL:VS03E_CAL.DAT'. Output sent to TY(1) and GC(1). For Halca, used a nominal Tsys' values of 95K, 98K for IF1, IF2. Shifted two Tsys values for Sh by 5 minutes so ANTAB would apply them. 
APCAL
 
 
 
Input: Ty(1) + GC(1) 
SNSMO
 
 
 
 
Did not use 
CLCAL OPCODE = CALI
INTERPOL = 2PT
REFANT 2 (Sechan)
 
 
TACOP
 
 
 
CLCOR ANTENNAS=0
OPCODE=GAIN
CLCORPRM=0.9055
GAINVER=3
 
 
Correction for Van Vleck normalization. 
CLCOR OPCODE='SBDL'
ANTENNAS = 1 (Hart)
CLCORPRM= 164, 164
GAINVER=3
 
 
 
CLCOR OPCODE='SBDL'
ANTENNAS = 1 (Halca)
CLCORPRM= 158, 158
GAINVER=3
 
 
 
CLCOR OPCODE='SBDL'
ANTENNAS = 3 (Mopra)
CLCORPRM= -109, -109
GAINVER=3
 
 
 
FRING APARM(1)=2
APARM(7)=3 (SNR=3)
APARM(9)=1
DPARM(1)=1 (no baseline
   stacking)
DPARM(2)=300 (300ns delay
   window)
DPARM(3)=100 (100mHz rate
   window)
DPARM(4)=0.5 (0.5 sec integration
   time)
DPARM(6)=1 (don't average
   in frequency)
BCHAN 0, ECHAN 0
SEARCH 3
REFANT 2 (Seshan)
 
 
These are the standard parameters I used (unless otherwise specified). 
FRING Standard+
SOLINT=5
TIMER 0 18 30 0 0 19 0 0
DOCALIB 1, GAINUSE 3
 
 
Got good solutions (ground SNRs were on the order of 80, space-ground SNRs were on the order of 10). Abs(delay) less than 25ns, Abs(rate) less than 25mHz. 
FRING Standard+
SOLINT=5
DPARM(2)=200
DOCALIB 1, GAINUSE 3
 
 
Solutions look good. 
SNEDT
 
 
 
 
Did not use/need. 
CLCAL OPCODE='CALI'
INTERPOL = '2PT'
REFANT 2
 
 
CALIB
 
 
 
 
Not used. 
TASAV
 
 
 
 
Input file: VS03E.FIXWT, Output file: VS03E.TABLES 
SPLIT SOURCES 'J0405-13'
BCHAN 0, ECHAN 0
DOCALIB 1, GAINUSE 4
APARM(1)=2 (average each
   IF separately)
APARM(2)=0.5
APARM(4)=1
 
 
 
Input file: VS03E.FIXWT, Output file: J0405-13.FITS 
FITTP
 
 
 
 
Input file: VS03E.FITS, Output file: FITS:J0405-13.FITS 

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

Additional Files
NameDescription
image.ps.gzThe final Difmap image (gzipped).

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
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? Yes
Amplitude selfcal on non-global timescales used? No
Modelfit made and saved? Yes
Image Made and saved? Yes
Comments on Difmap processing
Ran uvaver 30,true (averaged over 30 seconds and redo the weights). Did not try amp-self-cal, since there were not enough antennas. Did not add any clean components outside of the core, since I could not tell if they were real, or sidelobes. Final image: Core was slightly resolved, with component in roughly a NNE-SSW direction. Peak core amplitude was 0.358 Jy/beam. There was possibly an additional component to the NE, although it was difficult to determine if it was real or not.

Image
Ampl, Phase vs (u,v) Distance
PS (28 kb)
JPEG (38 kb)
Ampl, Phase vs Time
PS (82 kb)
JPEG 1, 2
(u,v) Coverage
PS (15 kb)
JPEG (26 kb)
Closure Phase vs Time
PS (52 kb)
JPEG 1
Clean Image
PS (41 kb)
JPEG (44 kb)
Modelfit
Ampl, Phase vs (u,v) Distance
PS (28 kb)
JPEG (39 kb)
Ampl, Phase vs Time
PS (83 kb)
JPEG 1, 2
(u,v) Coverage
PS (15 kb)
JPEG (26 kb)
Closure Phase vs Time
PS (52 kb)
JPEG 1
Image with model components
PS (47 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)
0.411363 0.0123678 131.683 0.194289 1.00000 22.6356 0.5318
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



Last updated on Mon Nov 19 18:32:48 GMT 2001
by db_results.pl version 0.3.