EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EK020C_1. 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 27 16:36:53 CET 2006 bignall@jive.nl


General Comments. ( Brief data summary and scan listing )
Pipeline results for EK020C continuum pass. EK020C was recorded at 128 Mbps on 8 June 2005 (2 IFs, dual pol, correlated with 128 channels per IF).

Urumqi did not observe, and Noto could not observe due to an antenna problem.
Torun used Rubidium frequency standard.
Effelsberg lost the first 30 minutes, and Arecibo lost half of the scheduled time due to FS-Mk5 communication problems.
Jodrell has no good LCP data in IF #2 (spectral line is in IF #1)
No other problems apart from RFI.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.56 . ERI* = 0.56 . (EF=0.95, CM=1, NT=0, TR=1, JB=0.88, WB=1, ON=1, MC=1, UR=0, HH=1, AR=0.5)


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 produced before self-cal of:
2134+004: postscript , or FITS .
J2139+1423: postscript , or FITS .
J2052+1619: postscript , or FITS .
I20550: postscript , or FITS .
3C286: postscript , or FITS .
Comments.


Uniformly weighted dirty map produced before self-cal of:
2134+004: postscript , or FITS .
J2139+1423: postscript , or FITS .
J2052+1619: postscript , or FITS .
I20550: postscript , or FITS .
3C286: postscript , or FITS .
Comments.


Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
2134+004.
J2139+1423.
J2052+1619.
I20550. (not available)
3C286.
Comments.


Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
2134+004: postscript , or text file , or statistical summary .
J2139+1423: postscript , or text file , or statistical summary .
J2052+1619: postscript , or text file , or statistical summary .
I20550: postscript (not available) , or text file (not available) , or statistical summary (not available) .
3C286: postscript , or text file , or statistical summary .
Comments.


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).
Comments.


Residual closure phase (visibility closure phase with model closure phase subtracted) for:
2134+004 .
J2139+1423 .
J2052+1619 .
I20550 (not available) .
3C286 .
Comments.


Calibrated visibilities and the source model of:
2134+004 .
J2139+1423 .
J2052+1619 .
I20550 (not available) .
3C286 .
Comments.


Calibrated visibilities against u,v distance for:
2134+004. postscript , or png (smaller)
J2139+1423. postscript , or png (smaller)
J2052+1619. postscript , or png (smaller)
I20550. postscript , or png (smaller)
3C286. postscript , or png (smaller)
Comments.


u,v coverage for:
2134+004. postscript , or png (smaller)
J2139+1423. postscript , or png (smaller)
J2052+1619. postscript , or png (smaller)
I20550. postscript , or png (smaller)
3C286. postscript , or png (smaller)
Comments.


Crude maps of sources:
2134+004: postscript , or FITS .
J2139+1423: postscript , or FITS .
J2052+1619: postscript , or FITS .
I20550: postscript , or FITS .
3C286: postscript , or FITS .
Comments.