VS03q Results
Submitted checklist.txt and checklist.tex is also available
  [Summary | AIPS | Difmap ]
Analyst: Zsolt Paragi
Date Prepared: 26-01-2001
 

Summary
 
Observation code : VS03q    AIPS Version : 15APR99   
Date of Observation : 1998/218    Difmap Version : 2.3c 
Source Name : J0339-0146    vsop_difmap used : No 
Calibration Source(s) : 0420-014         
Ground telescopes : CEDUNA, SESHAN25  Model Fitted to data : Yes 
Tracking Station(s) : TZ, RZ, UZ    Image made : Yes 
Correlator : Pentincton         

 
Abstract
Only two GRTs were in the experiment. Ceduna performance was bad between ~21h-23h UT. The source was not detected on the longest space baselines (23h-01h UT). Imaging was possible with phase-only calibration (HALCA provided some data on short spacings!). The correlated flux density at 100 Mlambda was a bit less than in the VLBApls dataset. The relative amplitude calibration between the telescopes was OK. The calibrator source was not splitted as the data were not enough for checking the absolute amplitude calibration. The source was resolved; a single Gaussian component was fitted to the data.
Model
Flux (Jy)
Radius (mas)
Theta (deg)
Major (mas)
Axial ratio
Phi (deg)
TB (10^12 K)
0.899008 0.0375950 59.8420 0.325436 0.579968 49.6938 0.7142
(*) 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 douvcomp 1
 
 
 
 
Data received on DAT tape from Leonid Gurvits (JIVE). 
FIXWT bif = 1
bchan = 100
detime = -1
 
 
 
 
 
INDXR cparm = 0, 0, 0.25, 0
 
 
 
Input scan break taken from PI letter. 
TABED bcount = 2
ecount = 3
keyval = 2
 
 
 
 
Correct antenna type for HALCA (MNTSTA: orbiter->2) 
ANTAB tyver = 1
gcver = 1
 
 
 
 
Gain curve information from VSOP calibration web page. Nominal Tsys used for Ceduna and HALCA. 
APCAL
 
 
 
 
CLCAL opcode = 'cali'
interpol = '2pt'
 
 
TACOP
 
 
 
CLCOR timer 1 1 18 0 1 1 48 15
opcode 'sbdl'
antennas 2 0
gainver 3
clcorprm -500, -500
 
 
Fringes were not found in the 3rd tracking pass. Shift HALCA delays by 500 ns-- this way the delay window may be decreased in FRING. 
FRING docalib = 1
flagver = 1
refant = 1
search = 1,3
solint = 5
aparm = 2, 0, 0, 0, 2, 1,
   4, 0, 1
dparm = 3, 400, 100, 0.7
 
 
Ceduna was not good reference antenna. 
FRING docalib = 1
flagver = 1
refant = 3
search = 3,1
solint = 5
aparm = 2, 0, 0, 0, 2, 1,
   4, 0, 1
dparm = 3, 400, 100, 0.7
 
 
Reference antenna was Shanghai. 
CLCAL opcode = 'cali'
interpol = 'ambg'
refant 3
 
 
TACOP
 
 
 
CLCOR opcode = 'gain'
antenn = 0
clcorprm = 0.906, 0
 
 
Gain correction for Penticton data correlated before 14 Feb 1999. 
SPLIT aparm = 2, 0.7, 0, 1, 0
sources 'J0339-01' ''
 
 
 
The calibrator source was not splitted. 
FITTP
 
 
 
 
Data written out for analysis in Difmap. 

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

Additional Files
NameDescription
processing.logAIPS data reduction log file with detailed notes.

AIPS Output Files
PRTAN.LIS
LISTR.LIS
DTSUM_0.LIS
DTSUM_1.LIS
UVPLT_UV.PS
UVPLT_UVD.PS
UVPLT_UVPA.PS
SN_APCAL_AMP_2.P
SN_APCAL_AMP_1.P
SN_CALIB_DEL_1.P
SN_CALIB_DEL_2.P
SN_CALIB_RAT_1.P
SN_CALIB_RAT_2.P
SN_CALIB_SNR_1.P
SN_CALIB_SNR_2.P
SN_CALIB_PHA_1.P
SN_CALIB_PHA_2.P
POSSM01_AP_1.PS
POSSM01_AP_2.PS
POSSM02_AP_1.PS
POSSM02_AP_2.PS
POSSM03_AP_1.PS
POSSM03_AP_2.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

Image
Ampl, Phase vs (u,v) Distance
PS (26 kb)
JPEG (40 kb)
Ampl, Phase vs Time
PS (105 kb)
JPEG 1, 2
(u,v) Coverage
PS (13 kb)
JPEG (25 kb)
Closure Phase vs Time
PS (57 kb)
JPEG 1
Clean Image
PS (38 kb)
JPEG (47 kb)
Modelfit
Ampl, Phase vs (u,v) Distance
PS (20 kb)
JPEG (39 kb)
Ampl, Phase vs Time
PS (97 kb)
JPEG 1, 2
(u,v) Coverage
PS (13 kb)
JPEG (25 kb)
Closure Phase vs Time
PS (56 kb)
JPEG 1
Image with model components
PS (825 bytes)
JPEG (0 bytes)

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)
0.899008 0.0375950 59.8420 0.325436 0.579968 49.6938 0.7142
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.



Last updated on Wed Jan 31 09:30:33 GMT 2001
by db_results.pl version 0.3.