EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EA033. If you have any comments on this experiment please email the address below.
A detailed description of the pipeline output is available.

Last updated: Mon Feb 13 15:34:43 CET 2006 soria@jive.nl

General Comments. ( Brief data summary and scan listing )
EA033 was observed on June 2005 (11 telescopes, 4 bands & 4 pols, dual polarizaton and 2-bit sampling), correlated with 16 spectral channels. Ef had some playback problems which affect the subband 0 data after 7:50 UT. RCP subband 1 missed in Tr due to BBC#3 being unlocked.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.90 . ERI* = 0.76 . (JB=1, WB=1, EF=0.97 , ON=1, MC=1, NT=0, TR=0.94 , SH=0.75 , UR=1, HH=1, CM=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 produced before self-cal of:
3C48: postscript , or FITS .
DA193: postscript , or FITS .
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Uniformly weighted dirty map produced before self-cal of:
3C48: postscript , or FITS .
DA193: postscript , or FITS .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C48.
DA193.
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C48: postscript , or text file , or statistical summary .
DA193: postscript , or text file , or statistical summary .
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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:
3C48 .
DA193 .
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Calibrated visibilities and the source model of:
3C48 .
DA193 .
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Calibrated visibilities against u,v distance for:
3C48. postscript , or png (smaller)
DA193. postscript , or png (smaller)
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u,v coverage for:
3C48. postscript , or png (smaller)
DA193. postscript , or png (smaller)
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Crude maps of sources:
3C48: postscript , or FITS .
DA193: postscript , or FITS .
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