EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EM059A. If you have any comments on this experiment please email the address below.
A detailed description of the pipeline output is available.

Last updated: Tue Feb 14 13:09:47 CET 2006 bignall@jive.nl

General Comments. ( Brief data summary and scan listing )
EM059A is a 22 GHz phase-referencing experiment observed on 26 October 2005 at 128 Mbps (one 16MHz IF, dual polarization, 2-bit sampling). Correlation produced 1024 spectral channels and 2s integration time.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.66 . ERI* = 0.66 . (EF=1, JB=1, ON=0.93, MC=1, SH=0, MH=0.85, UR=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 produced before self-cal of:
2007+402: postscript , or FITS .
2015+3710: postscript , or FITS .
2007+777: postscript , or FITS .
IRAS2012: postscript , or FITS .
2002+472: postscript , or FITS .
Comments.

Uniformly weighted dirty map produced before self-cal of:
2007+402: postscript , or FITS .
2015+3710: postscript , or FITS .
2007+777: postscript , or FITS .
IRAS2012: postscript , or FITS .
2002+472: postscript , or FITS .
Comments.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
2007+402.
2015+3710.
2007+777.
IRAS2012. (not available)
2002+472.
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
2007+402: postscript , or text file , or statistical summary .
2015+3710: postscript , or text file , or statistical summary .
2007+777: postscript , or text file , or statistical summary .
IRAS2012: postscript (not available) , or text file (not available) , or statistical summary (not available) .
2002+472: 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:
2007+402 .
2015+3710 .
2007+777 .
IRAS2012 (not available) .
2002+472 (not available) .
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Calibrated visibilities and the source model of:
2007+402 .
2015+3710 .
2007+777 .
IRAS2012 (not available) .
2002+472 (not available) .
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Calibrated visibilities against u,v distance for:
2007+402. postscript , or png (smaller)
2015+3710. postscript , or png (smaller)
2007+777. postscript , or png (smaller)
IRAS2012. postscript , or png (smaller)
2002+472. postscript (not available) , or png (smaller) (not available)
Comments.

u,v coverage for:
2007+402. postscript , or png (smaller)
2015+3710. postscript , or png (smaller)
2007+777. postscript , or png (smaller)
IRAS2012. postscript , or png (smaller)
2002+472. postscript (not available) , or png (smaller) (not available)
Comments.

Crude maps of sources:
2007+402: postscript , or FITS .
2015+3710: postscript , or FITS .
2007+777: postscript , or FITS .
IRAS2012: postscript , or FITS .
2002+472:postscript (not available) , or FITS (not available) .
Comments.