EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EM095A. 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 13 12:54:58 CEST 2012 yang@jive.nl

General Comments. ( Brief data summary and scan listing )
C band phase-referencing e-VLBI experiment, observed on 1 Jun 2012. Data rate was 1 Gbps (8 X 16 MHz subbands, dual polarization, two-bit sampling). The target sources N4088-X1 and N4861-X2 were calibrated using the phase-reference sources J1203+4863 and J1308+3546, respectively. '4C39.25' was the fringe finder and the bandpass calibrator.
8 stations participated. Noto was limted to 512 Mbps.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.83 . ERI* = 0.83 . See PI Letter (JB=0.4, TR=0.94).

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 (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:
4C39.25: pdf (not available) , or FITS (not available) .
N4088-X1: pdf , or FITS .
J1203+4803: pdf (not available) , or FITS (not available) .
J1308+3546: pdf (not available) , or FITS (not available) .
N4861-X2: pdf , or FITS .
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Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
4C39.25: pdf (not available) , or FITS (not available) .
N4088-X1: pdf , or FITS .
J1203+4803: pdf (not available) , or FITS (not available) .
J1308+3546: pdf (not available) , or FITS (not available) .
N4861-X2: pdf , or FITS .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
4C39.25 .
N4088-X1 (not available) .
J1203+4803 .
J1308+3546 .
N4861-X2 (not available) .
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
4C39.25: pdf , or text file , or statistical summary .
N4088-X1: pdf (not available) , or text file (not available) , or statistical summary (not available) .
J1203+4803: pdf , or text file , or statistical summary .
J1308+3546: pdf , or text file , or statistical summary .
N4861-X2: 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:
4C39.25 .
N4088-X1 (not available) .
J1203+4803 .
J1308+3546 .
N4861-X2 (not available) .
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Calibrated visibilities and the source model of:
4C39.25 .
N4088-X1 (not available) .
J1203+4803 .
J1308+3546 .
N4861-X2 (not available) .
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Calibrated visibilities against u,v distance for:
4C39.25: pdf , or png .
N4088-X1: pdf , or png .
J1203+4803: pdf , or png .
J1308+3546: pdf , or png .
N4861-X2: pdf , or png .
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u,v coverage for:
4C39.25: pdf , or png .
N4088-X1: pdf , or png .
J1203+4803: pdf , or png .
J1308+3546: pdf , or png .
N4861-X2: pdf , or png .
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Crude maps of sources:
4C39.25: pdf , or FITS .
N4088-X1: pdf , or FITS .
J1203+4803: pdf , or FITS .
J1308+3546: pdf , or FITS .
N4861-X2: pdf , or FITS .
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