VS05t Results
Submitted checklist.txt and checklist.tex is also available |
[Summary | AIPS | Difmap ] |
Observation code | : | VS05t | AIPS Version | : | 15APR98 | |
Date of Observation | : | 1997/339 | Difmap Version | : | 2.3c | |
Source Name | : | J1037-2934 | vsop_difmap used | : | No | |
Calibration Source(s) | : | 1156+295 | ||||
Ground telescopes | : | CD, HA | Model Fitted to data | : | No | |
Tracking Station(s) | : | TZ, GZ | Image made | : | No | |
Correlator | : | Pentictn |
Abstract
This is one of "two GRT experiments". The data was originaly examined at the 1st Survey Data Reduction Meeting in April 98 by Gurvits and Horiuchi. Fringes were found only CD-HA baseline. The CD has no fringes in IF2. There is no time to satisfy the phase clousre with three baselines, hence no self-cal has been performed. The source seems to show a small extended structure according to other groud only observations. Amplitude vs. uv-distant plot for our CD-HA baseline shows a variation of visibilities 0.4-0.8 Jy upto 150Mlambda. Better uv coverage ensures the ideal VSOP survey results with some fine scale images. The observations of this source should be re-scheduled. |
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FITLD |
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Files can not be concatinated because of wrong obs. date. | |
INDXR |
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FRING | Solint=1, APARM(7)=3, DPARM=1,16000,1000,0, REFANT=3 |
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No space fringes. No Ceduna fringes in IF2. |
ANTAB |
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APCAL |
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CLCAL | SMOTYPE = 'AMPL' |
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CLCAL | SMOTYPE = 'VLBI' |
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SPLIT |
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FITTP |
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AIPS Input Files
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
No imaging has been made. |