Logged on 08/24/2009 05:40:44 PM
This time the source is linearly polarised with an angle or 45'. I = 10Jy, U = 10Jy
Logged on 08/24/2009 05:52:09 PM
The MS was simulated as in the previous challenge, and a dirty image was generated. The source can be seen in stokes I and U. Q and V contain an image which looks similar to when the model was subtracted from uncalibrated data in challenge 1. This makes sense since Q and V are related to the difference of the X and Y feeds.
SSSC7_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 05:55:36 PM
Subtracting the model from the uncalibrated data gives the expected results. This time however the artifacts are visible in all stokes.
SSSC7_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 06:04:15 PM
Calibrating using G Jones yields good residual images.
SSSC7_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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