EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EC022. 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 Nov 11 12:57:22 CET 2004 brunthaler@jive.nl

General Comments. ( Brief data summary and scan listing )
5 GHz continuum experiment, recorded at 128 Mbps on 26 May 2004. There are 2 polarisations and two 8 GHz subbands, with 16 channels per subband. Participating stations were NT, SH, TR, MC, EF, WB, ON, JB, UR. The EVN reliability indicator (ERI) for this experiment was ERI=ERI*=

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:
1739+522: postscript , or FITS .
J1421+4645: postscript , or FITS .
J1800+7828: postscript , or FITS .
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Uniformly weighted dirty map produced before self-cal of:
1739+522: postscript , or FITS .
J1421+4645: postscript , or FITS .
J1800+7828: postscript , or FITS .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
1739+522.
J1421+4645.
J1800+7828.
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
1739+522: postscript , or text file .
J1421+4645: postscript , or text file .
J1800+7828: postscript , or text file .
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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:
1739+522 .
J1421+4645 .
J1800+7828 .
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Calibrated visibilities and the source model of:
1739+522 .
J1421+4645 .
J1800+7828 .
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Calibrated visibilities against u,v distance for:
1739+522. postscript , or png (smaller)
J1421+4645. postscript , or png (smaller)
J1800+7828. postscript , or png (smaller)
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u,v coverage for:
1739+522. postscript , or png (smaller)
J1421+4645. postscript , or png (smaller)
J1800+7828. postscript , or png (smaller)
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1739+522: postscript , or FITS .
J1421+4645: postscript , or FITS .
J1800+7828: postscript , or FITS .
Comments.