EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EM059B. 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 Jul 27 13:56:27 CEST 2007 soria@jive.nl

General Comments. ( Brief data summary and scan listing )
EM059B was observed on the 6th of March 2007. The experiment was processed with the following parameters: 8 Tels, 1 band X 2 pols, each with 1024 points, 2 sec int. The target source IRAS2012 was calibrated using the phase-reference source 2007+402. 2002+472 was the fringe finder.
7 stations participated in the experiment.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.97 . ERI* = 0.97 . (EF=0.89, MC=1, ON=1, MH=1, NT=1, JB=1, SH=1)

Plots of the autocorrelations
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1848 pages

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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1392 pages

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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530 pages

Naturally weighted dirty map (not useful for bright sources) produced before self-cal of:
2007+777: pdf (not available) , or FITS (not available) .
2002+472: pdf (not available) , or FITS (not available) .
2015+3710: pdf (not available) , or FITS (not available) .
2007+402: pdf (not available) , or FITS (not available) .
IRAS2012: pdf , or FITS .
Comments.

Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
2007+777: pdf (not available) , or FITS (not available) .
2002+472: pdf (not available) , or FITS (not available) .
2015+3710: pdf (not available) , or FITS (not available) .
2007+402: pdf (not available) , or FITS (not available) .
IRAS2012: pdf , or FITS .
Comments.

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

u,v coverage for:
2007+777: pdf , or png .
2002+472: pdf , or png .
2015+3710: pdf , or png .
2007+402: pdf , or png .
IRAS2012: pdf , or png .
Comments.

Crude maps of sources:
2007+777: pdf , or FITS .
2002+472: pdf , or FITS .
2015+3710: pdf , or FITS .
2007+402: pdf , or FITS .
IRAS2012: pdf , or FITS .
Comments.