EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment RT006B. 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 Dec 7 10:33:05 CET 2009 zparagi@jive.nl

General Comments. ( Brief data summary and scan listing )
C-band e-VLBI run on 13 November 2008 at 512 Mbps. Participating telescopes were Ar, Cm(+Kn), Ef, Jb2, Mc, On, Tr and Wb.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.74 . ERI* = 0.85 . (Ar=0.98, Cm=0.7, Kn=0.7, Ef=0.94, Jb2=1, Mc=1, On=1, Tr=0.5/1, 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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Cm and Kn signal in IF2.

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:
J1911+1611: pdf (not available) , or FITS (not available) .
J1912+0518: pdf (not available) , or FITS (not available) .
J2002+4725: pdf (not available) , or FITS (not available) .
OQ208: pdf (not available) , or FITS (not available) .
SS433: pdf , or FITS .
Comments.

Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
J1911+1611: pdf (not available) , or FITS (not available) .
J1912+0518: pdf (not available) , or FITS (not available) .
J2002+4725: pdf (not available) , or FITS (not available) .
OQ208: pdf (not available) , or FITS (not available) .
SS433: pdf , or FITS .
Comments.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1911+1611 .
J1912+0518 .
J2002+4725 .
OQ208 .
SS433 (not available) .
Comments.

Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1911+1611: pdf , or text file , or statistical summary .
J1912+0518: pdf , or text file , or statistical summary .
J2002+4725: pdf , or text file , or statistical summary .
OQ208: pdf , or text file , or statistical summary .
SS433: pdf (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:
J1911+1611 .
J1912+0518 .
J2002+4725 .
OQ208 .
SS433 (not available) .
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Calibrated visibilities and the source model of:
J1911+1611 .
J1912+0518 .
J2002+4725 .
OQ208 .
SS433 (not available) .
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Calibrated visibilities against u,v distance for:
J1911+1611: pdf , or png .
J1912+0518: pdf , or png .
J2002+4725: pdf , or png .
OQ208: pdf , or png .
SS433: pdf , or png .
Comments.

u,v coverage for:
J1911+1611: pdf , or png .
J1912+0518: pdf , or png .
J2002+4725: pdf , or png .
OQ208: pdf , or png .
SS433: pdf , or png .
Comments.

Crude maps of sources:
J1911+1611: pdf , or FITS .
J1912+0518: pdf , or FITS .
J2002+4725: pdf , or FITS .
OQ208: pdf , or FITS .
SS433: pdf , or FITS .
Comments.