EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EK022A. 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 Feb 16 14:43:21 CET 2006 harvey@jive.nl

General Comments. ( Brief data summary and scan listing )
Wb had major problems with the 1Gbps recording in this session, which left the target sources with less time producing good data for this station. We have now fixed this problem for future observing runs.Mc also didn't have enough bandwidth to handle the full 1Gbps observations and experienced RFI.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.845 . ERI* = 0.845 . (WB=0.675, MC=0.75, UR=0.85, EF=0.81, SH=0.83, JB=1, TR=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 (not available) .
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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:
:postscript (not available) , or FITS (not available) .
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Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
:postscript (not available) , or FITS (not available) .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
. (not available)
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
: postscript (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:
(not available) .
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Calibrated visibilities and the source model of:
(not available) .
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Calibrated visibilities against u,v distance for:
. postscript (not available) , or png (smaller) (not available)
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u,v coverage for:
. postscript (not available) , or png (smaller) (not available)
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Crude maps of sources:
:postscript (not available) , or FITS (not available) .
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