VS04V1 Results
Submitted checklist.txt and checklist.tex is also available |
[Summary | AIPS | Difmap ] |
Observation code | : | VS04V1 | AIPS Version | : | 31DEC03 | |
Date of Observation | : | 2002/151 | Difmap Version | : | 2.4a | |
Source Name | : | J0303-62 | vsop_difmap used | : | No | |
Calibration Source(s) | : | J0450-81 | ||||
Ground telescopes | : | HH MP | Model Fitted to data | : | No | |
Tracking Station(s) | : | UZ | Image made | : | No | |
Correlator | : | Penticton |
Abstract
No GRT fringes till the end of the space tracking. It seems that the problem is with HH, so all that can be said is there were no space fringes in a single baseline. Not imaged (obviously). Unresolved on PTI (1.8 Jy) pretty constant in the ATCA monitoring (2.2 Jy). It is a ICRF source. We find 0.4 Jy. I think this makes it a failed experiment. |
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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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ACCOR | solint 5 |
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CLCAL | refant=1; |
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Amplitude calibration solutions applied. Hart as ref |
FRING | docal -1; dparm 2,400,400,0.5,0;aparm(7)=0.1;solint 5,10,15 |
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No fringes between VSOP and any. Hart-Mop before 7:30 |
CLCAL | refant=1; |
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FRING | ref 2; |
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FRING | ref 1;dparm 2 0 0 0.5;solint 5 10 |
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FRING | ref 2;dparm 2 0/400 0/400 0.5;aparm(5)=1;dparm(9)=1 |
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SNEDT/CLCAL | refant=2; |
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KRING | timer 0 7 12 0 0 7 30 0; dofit 3 |
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overlap regoin |
SPLIT | aparm(1)=2 0; |
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Av within IF |
FITTP |
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Data written out for analysis in Difmap |
AIPS Input Files
ANTAB.TXT | Comments dramatic change in the HH phase cal around when fringes appear. |
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
no image made. Flux is 0.4 This seems low, Mopra still down by ~ 4? |