EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment RR010. If you have any comments on this experiment please email the address below.
A detailed description of the pipeline output is available.

Last updated: Thu Jul 3 17:36:41 CEST 2014 zparagi@jive.nl

General Comments. ( Brief data summary and scan listing )
RR010, C-band e-VLBI ToO run on 2014 Jun 24. Participating telescopes were Effelsberg, Jodrell Bank 2, Noto, Onsala, Shanghai, Torun, Yebes and Westerbork. Bad weather accross Europe, thunderstorm at Ys (high Tsys-low sensitivity) and Ef (telescope stowed between ~14:30-15:15 UT). Nt had a problem with the cooling at the beginning, back to observing at ~15:50 UT. Jb2 also had very low sensitivity during the run.

The target SN2014BC was phase-referenced to J1219+4829. Amplitude check source was J1203+4803.


The EVN reliability indicator (ERI) for this experiment was ERI = 0.70 . ERI* = 0.84 . (Ef=0.875/1, Wb=1, Jb2=0.5, On=1, Nt=0.4, Tr=1, Ys=1, Sh=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:
J1203+4803: pdf (not available) , or FITS (not available) .
J1219+4829: pdf (not available) , or FITS (not available) .
1156+295: pdf (not available) , or FITS (not available) .
SN2014BC: pdf , or FITS .
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Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
J1203+4803: pdf (not available) , or FITS (not available) .
J1219+4829: pdf (not available) , or FITS (not available) .
1156+295: pdf (not available) , or FITS (not available) .
SN2014BC: pdf , or FITS .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1203+4803 .
J1219+4829 .
1156+295 .
SN2014BC (not available) .
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1203+4803: pdf , or text file , or statistical summary .
J1219+4829: pdf , or text file , or statistical summary .
1156+295: pdf , or text file , or statistical summary .
SN2014BC: 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:
J1203+4803 .
J1219+4829 .
1156+295 .
SN2014BC (not available) .
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Calibrated visibilities and the source model of:
J1203+4803 .
J1219+4829 .
1156+295 .
SN2014BC (not available) .
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Calibrated visibilities against u,v distance for:
J1203+4803: pdf , or png .
J1219+4829: pdf , or png .
1156+295: pdf , or png .
SN2014BC: pdf , or png .
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u,v coverage for:
J1203+4803: pdf , or png .
J1219+4829: pdf , or png .
1156+295: pdf , or png .
SN2014BC: pdf , or png .
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Crude maps of sources:
J1203+4803: pdf , or FITS .
J1219+4829: pdf , or FITS .
1156+295: pdf , or FITS .
SN2014BC: pdf , or FITS .
Comments.