EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment ER034. 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 Sep 26 09:20:47 CEST 2013 yang@jive.nl

General Comments. ( Brief data summary and scan listing )
K band EVN user experiment, observed on 12 Jun 2013. Data rate was 1 Gbps (8 X 16 MHz subbands, dual polarization, two-bit sampling). The target sources are quite bright so that they were calibrated by themself.
13 stations were requested. See the PI letter for more details.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.52 . ERI* = 0.52 . (BD=0, SV=0, NT=0.5, MH=0)

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:
3C454.3: pdf (not available) , or FITS (not available) .
1633+382: pdf (not available) , or FITS (not available) .
BLLAC: pdf (not available) , or FITS (not available) .
1803+784: pdf (not available) , or FITS (not available) .
Comments.

Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
3C454.3: pdf (not available) , or FITS (not available) .
1633+382: pdf (not available) , or FITS (not available) .
BLLAC: pdf (not available) , or FITS (not available) .
1803+784: pdf (not available) , or FITS (not available) .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C454.3 .
1633+382 .
BLLAC .
1803+784 .
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C454.3: pdf , or text file , or statistical summary .
1633+382: pdf , or text file , or statistical summary .
BLLAC: pdf , or text file , or statistical summary .
1803+784: pdf , or text file , or statistical summary .
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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:
3C454.3 .
1633+382 .
BLLAC .
1803+784 .
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Calibrated visibilities and the source model of:
3C454.3 .
1633+382 .
BLLAC .
1803+784 .
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Calibrated visibilities against u,v distance for:
3C454.3: pdf , or png .
1633+382: pdf , or png .
BLLAC: pdf , or png .
1803+784: pdf , or png .
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u,v coverage for:
3C454.3: pdf , or png .
1633+382: pdf , or png .
BLLAC: pdf , or png .
1803+784: pdf , or png .
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Crude maps of sources:
3C454.3: pdf , or FITS .
1633+382: pdf , or FITS .
BLLAC: pdf , or FITS .
1803+784: pdf , or FITS .
Comments.