Logged on 08/24/2009 03:14:09 PM
The source is simulated again but this time it is fully linearly polarised I = 10Jy, Q = 10Jy.
Logged on 08/24/2009 03:25:01 PM
The MS was simulated as in Challenge 1. A dirty image was generated, this time all 4 stokes were imaged and the image is visible in I and Q. U and V are blank meaning that there is no polarisation leakage.
SSSC6_WSRT.MS.DATA.channel.1ch.fits (header) 1x4x512x512 FITS cube, 4 planes are given below. | ||||||||||||||
Image plane #0.
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Image plane #1.
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Image plane #2.
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Image plane #3.
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Logged on 08/24/2009 04:23:56 PM
Subtracting the model from the uncalibrated data shows similar artifacts to in Challenge 1.
SSSC6_WSRT.MS.CORRECTED_DATA.channel.1ch.fits (header) 1x4x512x512 FITS cube, 4 planes are given below. | ||||||||||||||
Image plane #0.
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Image plane #1.
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Image plane #2.
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Image plane #3.
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Logged on 08/24/2009 04:30:26 PM
'Calibrate' and 'Correct data or residuals' as well as G Jones were selected in the TDL options and recompiled. The G diagonal terms were then calibrated and a residual image made. The residual image has a very low noise level, and the amplitudes are flat in the Corrected_data column. There does seem to be some artifact present however - a quite large almost horizontal ripple...
SSSC6_WSRT.MS.CORRECTED_DATA.channel.1ch.fits (header) 1x4x512x512 FITS cube, 4 planes are given below. | ||||||||||||||
Image plane #0.
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Image plane #1.
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Image plane #2.
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Image plane #3.
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