VS04v Results
Submitted checklist.txt and checklist.tex is also available |
[Summary | AIPS | Difmap ] |
Observation code | : | VS04v | AIPS Version | : | 15OCT98 | |
Date of Observation | : | 1998/157 | Difmap Version | : | 2.3c | |
Source Name | : | J0303-62 | vsop_difmap used | : | Yes | |
Calibration Source(s) | : | |||||
Ground telescopes | : | HartRAO, Mop | Model Fitted to data | : | No | |
Tracking Station(s) | : | RZ | Image made | : | No | |
Correlator | : | Penticton |
Abstract
This is a 2 GRTs experiment. No fringes were found on sapce baselines. A correlated flux density of ~0.2-0.6Jy was seen on the ground baseline (HartRAO -- Mop) of 9,000km in length. A re-scheduling is recommended! |
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FITLD | douvcomp=1;dotable=1 |
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load the uv FITS data into AIPS |
MSORT | sort='TB' |
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sort the data to 'TB' order |
INDXR | cparm(3)=1 |
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index uv data with 1 min CL entry interval |
TACOP |
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protect original CL1 | |
ANTAB |
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determine the Tsys and gain curve (see ANTAB.TXT file). Tsys=95K for Halca. | |
APCAL | opcode=' ' |
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generate an amplitude calibration solution table |
CLCAL | opcode='CALI' smotype='ampl' refant=0 |
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apply amplitude calibration solution |
FRING | docalib=1 flagv=-1;solint=4;refant=1 aparm=2,0,0,0,0,1,2,0 dparm=1,500,500,0 antwt=1,1,30 |
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try different searching windows and SNR cutoffs (no space fringes were found) |
CLCAL | opcode='CALP';interpol='ambg smotype='VLBI';refant=1 |
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apply FFT solutions |
TACOP |
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save calibration table CL4 | |
CLCOR | antenna=0;opcode='GAIN';clcorprm=0.91,0 |
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Penticton gain correction |
TASAV |
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copy all extension tables to a dummy file | |
SPLIT | docalib=1;douvcomp=1 flagv=-1;aparm=2,0,0,1,0 |
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make calibrated single-source data file: J0303-62.SPLIT |
AIPS Input Files
INDXR.TXT 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
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