EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EF023B. If you have any comments on this experiment please email the address below.
A detailed description of the pipeline output is available.

Last updated: Wed Jan 18 13:55:51 CET 2012 zparagi@jive.nl

General Comments. ( Brief data summary and scan listing )
L-band regular-VLBI short experiment. Participating telescopes were Ef, Wb, Jb1, On, Mc, Tr, Sv, Zc. Bd, Ur and Sh. Medicina had a recording problem. The target was phase-referenced to J1422+3223.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.76 . ERI* = 0.76 . (Ef=1, Wb=1, Jb1=0.75, Mc=0, On=1, Tr=0.88, Sv=1, Zc=1, Bd=1, Ur=1, Sh=1)

Plots of the autocorrelations
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RFI!

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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Tr: L5-6 dead (both related to BBC#6).

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 (not useful for bright sources) produced before self-cal of:
J1422+3223: pdf (not available) , or FITS (not available) .
J1425+3231: pdf , or FITS .
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Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
J1422+3223: pdf (not available) , or FITS (not available) .
J1425+3231: pdf , or FITS .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1422+3223 .
J1425+3231 (not available) .
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
J1422+3223: pdf , or text file , or statistical summary (not available) .
J1425+3231: 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:
J1422+3223 .
J1425+3231 (not available) .
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Calibrated visibilities and the source model of:
J1422+3223 .
J1425+3231 (not available) .
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Calibrated visibilities against u,v distance for:
J1422+3223: pdf , or png .
J1425+3231: pdf , or png .
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u,v coverage for:
J1422+3223: pdf , or png .
J1425+3231: pdf , or png .
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Crude maps of sources:
J1422+3223: pdf , or FITS .
J1425+3231: pdf , or FITS .
Comments.