EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EG069E. 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 Oct 31 13:18:52 CET 2013 zparagi@jive.nl

General Comments. ( Brief data summary and scan listing )
EG069E, C-band e-VLBI run on 2013 September 17. Participating telescopes were Jodrell Bank (MkII), Westerbork, Effelsberg, Onsala, Medicina, Noto, Torun, and Yebes. Medicina observed at 512 Mbps (but used 1-bit sampling to recover the full bandwidth). Torun had no RCP fringes in the last two RCP subbands.

The target and check sources were phase referenced to J1818+5017.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.98 . ERI* = 0.98 . (Ef=1, Jb2=1, Ys=1, On=1, Mc=1, Nt=1, Tr=0.91, 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
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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:
J1809+5007: pdf , or FITS .
1823+568: pdf (not available) , or FITS (not available) .
AMHER: pdf , or FITS .
1308+326: pdf (not available) , or FITS (not available) .
J1818+5017: pdf (not available) , or FITS (not available) .
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Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
J1809+5007: pdf , or FITS .
1823+568: pdf (not available) , or FITS (not available) .
AMHER: pdf , or FITS .
1308+326: pdf (not available) , or FITS (not available) .
J1818+5017: pdf (not available) , or FITS (not available) .
Comments.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1809+5007 (not available) .
1823+568 .
AMHER (not available) .
1308+326 .
J1818+5017 .
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1809+5007: pdf (not available) , or text file (not available) , or statistical summary (not available) .
1823+568: pdf , or text file , or statistical summary .
AMHER: pdf (not available) , or text file (not available) , or statistical summary (not available) .
1308+326: pdf , or text file , or statistical summary .
J1818+5017: pdf , or text file , or statistical summary .
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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On between 12-14 UT low sensitivity because of rain?
Wb also lower sensitivity compared to nominal 60 Jy

Residual closure phase (visibility closure phase with model closure phase subtracted) for:
J1809+5007 (not available) .
1823+568 .
AMHER (not available) .
1308+326 .
J1818+5017 .
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Calibrated visibilities and the source model of:
J1809+5007 (not available) .
1823+568 .
AMHER (not available) .
1308+326 .
J1818+5017 .
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Calibrated visibilities against u,v distance for:
J1809+5007: pdf , or png .
1823+568: pdf , or png .
AMHER: pdf , or png .
1308+326: pdf , or png .
J1818+5017: pdf , or png .
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u,v coverage for:
J1809+5007: pdf , or png .
1823+568: pdf , or png .
AMHER: pdf , or png .
1308+326: pdf , or png .
J1818+5017: pdf , or png .
Comments.

Crude maps of sources:
J1809+5007: pdf , or FITS .
1823+568: pdf , or FITS .
AMHER: pdf , or FITS .
1308+326: pdf , or FITS .
J1818+5017: pdf , or FITS .
Comments.