VS13B Results
Submitted checklist.txt and checklist.tex is also available |
[Summary | AIPS | Difmap ] |
Observation code | : | VS13B | AIPS Version | : | 31DEC03 | |
Date of Observation | : | 2002/239 | Difmap Version | : | 2.4a | |
Source Name | : | J0414+05 | vsop_difmap used | : | No | |
Calibration Source(s) | : | J0423-01 | ||||
Ground telescopes | : | HO HH SH | Model Fitted to data | : | No | |
Tracking Station(s) | : | UZ | Image made | : | No | |
Correlator | : | Penticton |
Abstract
No fringes on long baselines - only SH-KA. This is a double with separation of 430 mas From pls: A gravitational lens with an overall size of 2.2" (e.g. Katz, Moore & Hewitt 1997). Two of the four lensed components are in our field of view, separated by ~430 mas (Figure 4). See Porcas (1998) and Trotter, Winn & Hewitt (2000) for recent 5 GHz VLBI images of this system. The prelaunch model resolves, and matches the survey data. |
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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. SH as ref |
FRING | docal -1;dparm 2,0,0,0.5,0;aparm(7)=0.1;solint 5,10,15 |
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Full range searched |
UVFIX/FRING | shift -0.1,0.9 |
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shift to the centre as seen on the short baseline. |
FRING | refa=3;dparm 2,0,0,0.5,0;aparm(7)=0.1;solint 5,10,15 |
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CLCAL | interp 'poly';intp 2; |
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SN#9 is just on the calibrator source |
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 - None - |
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
Nothing worth imaging |