EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment GB055A. 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 10:33:57 CET 2006 soria@jive.nl

General Comments. ( Brief data summary and scan listing )
GB055A was observed on October 2005 (16 telescopes, 4 bands & 2 pols), correlated with 16 spectral channels.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.63 . ERI* = 0.67 . (TR=0, ON=1, MC=1, JB=0.89, EF=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 (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:
3C345:postscript (not available) , or FITS (not available) .
J1310+322:postscript (not available) , or FITS (not available) .
J1337+550:postscript (not available) , or FITS (not available) .
MKN273: postscript , or FITS .
Comments.

Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
3C345:postscript (not available) , or FITS (not available) .
J1310+322:postscript (not available) , or FITS (not available) .
J1337+550:postscript (not available) , or FITS (not available) .
MKN273: postscript , or FITS .
Comments.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C345.
J1310+322.
J1337+550.
MKN273. (not available)
Comments.

Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C345: postscript , or text file , or statistical summary .
J1310+322: postscript , or text file , or statistical summary .
J1337+550: postscript , or text file , or statistical summary .
MKN273: postscript (not available) , or text file (not available) , or statistical summary (not available) .
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).
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Residual closure phase (visibility closure phase with model closure phase subtracted) for:
3C345 .
J1310+322 .
J1337+550 .
MKN273 (not available) .
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Calibrated visibilities and the source model of:
3C345 .
J1310+322 .
J1337+550 .
MKN273 (not available) .
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Calibrated visibilities against u,v distance for:
3C345. postscript , or png (smaller)
J1310+322. postscript , or png (smaller)
J1337+550. postscript , or png (smaller)
MKN273. postscript , or png (smaller)
Comments.

u,v coverage for:
3C345. postscript , or png (smaller)
J1310+322. postscript , or png (smaller)
J1337+550. postscript , or png (smaller)
MKN273. postscript , or png (smaller)
Comments.

Crude maps of sources:
3C345: postscript , or FITS .
J1310+322: postscript , or FITS .
J1337+550: postscript , or FITS .
MKN273: postscript , or FITS .
Comments.