EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment RSF05. If you have any comments on this experiment please email the address below.
A detailed description of the pipeline output is available.


Last updated: Fri Jan 13 16:32:48 CET 2012 zparagi@jive.nl


General Comments. ( Brief data summary and scan listing )
RSF05, C-band short e-VLBI run on 2012 Jan. 10. Participating telescopes were Jodrell Bank (MkII), Westerbork, Effelsberg, Onsala, Medicina, Torun and Hartebeesthoek. Yebes could not take part because of a Makr5B problem. Shanghai data were lost for RSF05 because of a temporary network outage in Canada. The target J0648+1516 was phase-referenced to J0637+1458.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.67 . ERI* = 0.9 . (Ef=0.75, Jb2=1, Mc=1, On=1, Tr=0.88, Wb=1, Hh=1, Sh=0/1)


Plots of the autocorrelations
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plots of the uncalibrated amplitude and phase against time
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Plots of the uncalibrated amplitude and phase against frequency channel
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Ef: DBBC problems; used Mark5A on MkIV rack, but this limited the data rate to 768 Mbps.
Tr: IFs L5-6 missing (BBC#6 dead)


The uncalibrated amplitude and phase of the crosshand correlations against frequency channel
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TSYS against time
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Telescope sensitivities from the a priori TSYS and Gain curves (the square of this number gives the antenna noise (SEFD) in Jy - the smaller the better).
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Fringe-fit phase solutions (including Parallactic Angle correction).
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Fringe-fit delay solutions
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Fringe-fit rate solutions
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Telescope bandpasses
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Calibrated amplitude and phase against time (a priori amplitude calibration and fringe-fit solutions applied).
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Calibrated amplitude and phase against frequency channel
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Naturally weighted dirty map (not useful for bright sources) produced before self-cal of:
J0637+1458: pdf (not available) , or FITS (not available) .
J0648+1516: pdf , or FITS .
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Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
J0637+1458: pdf (not available) , or FITS (not available) .
J0648+1516: pdf , or FITS .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J0637+1458 .
J0648+1516 (not available) .
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J0637+1458: pdf , or text file , or statistical summary (not available) .
J0648+1516: pdf (not available) , or text file (not available) , or statistical summary (not available) .
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Telescope sensitivities (the total AMP gain applied during both a priori and self calibration; the square of this number gives the antenna noise (SEFD) in Jy).
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Residual closure phase (visibility closure phase with model closure phase subtracted) for:
J0637+1458 .
J0648+1516 (not available) .
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Calibrated visibilities and the source model of:
J0637+1458 .
J0648+1516 (not available) .
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Calibrated visibilities against u,v distance for:
J0637+1458: pdf , or png .
J0648+1516: pdf , or png .
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u,v coverage for:
J0637+1458: pdf , or png .
J0648+1516: pdf , or png .
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Crude maps of sources:
J0637+1458: pdf , or FITS .
J0648+1516: pdf , or FITS .
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