VS10J1 Results
Submitted checklist.txt and checklist.tex is also available |
[Summary | AIPS | Difmap ] |
Observation code | : | VS10J1 | AIPS Version | : | 31DEC03 | |
Date of Observation | : | 2002/139 | Difmap Version | : | 2.4a | |
Source Name | : | J2341-58 | vsop_difmap used | : | No | |
Calibration Source(s) | : | J1617-77,J0303-62 | ||||
Ground telescopes | : | HH HO MO | Model Fitted to data | : | No | |
Tracking Station(s) | : | UZ | Image made | : | No | |
Correlator | : | Penticton |
Abstract
Mopra never tracked the source. HH & HO have fringes for the Cal sources, but nothing to the target. Source must resolve on GRT baselines. Mopra would have been useful. |
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FITLD | clint = 0.25 digicor = -1 delcorr = -1 |
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INDXR | cparm = 0, 0, 0.25; |
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ANTAB | infile='antab.txt' |
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APCAL |
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CLCAL | refant=1; |
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Amplitude calibration solutions applied. |
FRING | docal -1; dparm 2,400,400,0.5,0;aparm(7)=0.1;solint 5,10,15 |
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FRING | dparm 2,0,0,0.5,0;refa 3/2;solint 5;cals '-J2341-58''/'' |
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Do get fringes HH to HO for calibration sources (#6) |
UVFLG | ante 3;flagv 1; |
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No Mopra |
FRING | flagv 1;dparm 2 50/-1 50 0.5 0;solint 10;aparm(5)=0/1 |
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Try try again. Hints at the start (shortest GRT), but nothing we could use amplitude |
AIPS Input Files
ANTAB.TXT | Comments used nominal_tsys.pl |
AIPS Output Files
Phase selfcal applied? | No |
Global amplitude selfcal (gscal) applied? | No |
Amplitude selfcal on non-global timescales used? | No |
Modelfit made and saved? | No |
Image Made and saved? | No |
Comments on Difmap processing
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