EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment RSC02. 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 Nov 21 15:56:48 CET 2014 zparagi@jive.nl

General Comments. ( Brief data summary and scan listing )
RSC02, C-band short e-VLBI experiment on 2014 November 18. Participating telescopes were Effelsberg, Jodrell Bank (MkII), Noto, Onsala, Shanghai, Torun, Yebes and Westerbork (Medicina was not scheduled because of an antenna problem). Jodrell MkII pointing error is now fixed.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.98 . ERI* = 0.98 . (Ef=1, Ys=1, Jb2=1, Sh=1, On=1, Nt=0.94, Tr=1, Wb=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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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:
J0753+5352: pdf (not available) , or FITS (not available) .
J0809+5341: pdf (not available) , or FITS (not available) .
J0807+5117: pdf (not available) , or FITS (not available) .
J0809+5218: pdf (not available) , or FITS (not available) .
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Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
J0753+5352: pdf (not available) , or FITS (not available) .
J0809+5341: pdf (not available) , or FITS (not available) .
J0807+5117: pdf (not available) , or FITS (not available) .
J0809+5218: pdf (not available) , or FITS (not available) .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J0753+5352 .
J0809+5341 .
J0807+5117 .
J0809+5218 .
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J0753+5352: pdf (not available) , or text file (not available) , or statistical summary (not available) .
J0809+5341: pdf (not available) , or text file (not available) , or statistical summary (not available) .
J0807+5117: pdf (not available) , or text file (not available) , or statistical summary (not available) .
J0809+5218: pdf (not available) , or text file (not available) , or statistical summary (not available) .
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Telescope sensitivities (not available) (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:
J0753+5352 .
J0809+5341 .
J0807+5117 .
J0809+5218 .
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Calibrated visibilities and the source model of:
J0753+5352 .
J0809+5341 .
J0807+5117 .
J0809+5218 .
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Calibrated visibilities against u,v distance for:
J0753+5352: pdf , or png .
J0809+5341: pdf , or png .
J0807+5117: pdf , or png .
J0809+5218: pdf , or png .
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u,v coverage for:
J0753+5352: pdf , or png .
J0809+5341: pdf , or png .
J0807+5117: pdf , or png .
J0809+5218: pdf , or png .
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Crude maps of sources:
J0753+5352: pdf , or FITS .
J0809+5341: pdf , or FITS .
J0807+5117: pdf , or FITS .
J0809+5218: pdf , or FITS .
Comments.