EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment EC052C. 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 Feb 16 10:34:23 CET 2015 zparagi@jive.nl


General Comments. ( Brief data summary and scan listing )
EC052C, L-band e-VLBI experiment on 2015 February 10-11. Participating telescopes were Effelsberg, Hartebeesthoek, Jodrell Bank (MkII), Medicina, Onsala, Sheshan, Torun, and Westerbork. Medicina is back in the array, but still with the 512 Mbps - 1-bit limitation. Noto 18cm receiver upgrade not ready. Sheshan 18cm receiver was fixed just before the run; Sh was added to the array, but the observing schedule was not optimized for source visibility at Sh.

The following subands were flagged in this pipeline because they were corrupt/highly unstable due to strong RFI: Jb IF4, 5, 7; Mc IF1, 2, 8; Tr IF1; Wb IF2, 3. No antabfs file for Jb - a SEFD of ~860 Jy was used in this pipeline (cf. nominal 320 Jy). Sh provided no antabfs file either, nominal Sh 25m SEFD was used in this pipeline.

The targets 0011+1446, 0210-0018, 1013+2811 and 1311+2227 were phase-referenced to J0010+1724, J0216-0105, J1023+2856 and J1321+2216, respectively.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.56 . ERI* = 0.78 . (Ef=1, Hh=1, Jb2=0.625/1.0, On=1.0, Mc=0.625/1.0, Nt=0, Sh=1, Tr=0.875/1.0, Wb=0.75/1.0)


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:
OJ287: pdf (not available) , or FITS (not available) .
J0010+1724: pdf (not available) , or FITS (not available) .
0210-0018: pdf , or FITS .
J1023+2856: pdf (not available) , or FITS (not available) .
0011+1446: pdf , or FITS .
J0216-0105: pdf (not available) , or FITS (not available) .
1013+2811: pdf , or FITS .
J1321+2216: pdf (not available) , or FITS (not available) .
1311+2227: pdf , or FITS .
Comments.


Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
OJ287: pdf (not available) , or FITS (not available) .
J0010+1724: pdf (not available) , or FITS (not available) .
0210-0018: pdf , or FITS .
J1023+2856: pdf (not available) , or FITS (not available) .
0011+1446: pdf , or FITS .
J0216-0105: pdf (not available) , or FITS (not available) .
1013+2811: pdf , or FITS .
J1321+2216: pdf (not available) , or FITS (not available) .
1311+2227: pdf , or FITS .
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Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
OJ287 .
J0010+1724 .
0210-0018 (not available) .
J1023+2856 .
0011+1446 (not available) .
J0216-0105 .
1013+2811 (not available) .
J1321+2216 .
1311+2227 (not available) .
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Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
OJ287: pdf , or text file , or statistical summary .
J0010+1724: pdf , or text file , or statistical summary .
0210-0018: pdf (not available) , or text file (not available) , or statistical summary (not available) .
J1023+2856: pdf , or text file , or statistical summary .
0011+1446: pdf (not available) , or text file (not available) , or statistical summary (not available) .
J0216-0105: pdf , or text file , or statistical summary .
1013+2811: pdf (not available) , or text file (not available) , or statistical summary (not available) .
J1321+2216: pdf , or text file , or statistical summary .
1311+2227: 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:
OJ287 .
J0010+1724 .
0210-0018 (not available) .
J1023+2856 .
0011+1446 (not available) .
J0216-0105 .
1013+2811 (not available) .
J1321+2216 .
1311+2227 (not available) .
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Calibrated visibilities and the source model of:
OJ287 .
J0010+1724 .
0210-0018 (not available) .
J1023+2856 .
0011+1446 (not available) .
J0216-0105 .
1013+2811 (not available) .
J1321+2216 .
1311+2227 (not available) .
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Calibrated visibilities against u,v distance for:
OJ287: pdf , or png .
J0010+1724: pdf , or png .
0210-0018: pdf , or png .
J1023+2856: pdf , or png .
0011+1446: pdf , or png .
J0216-0105: pdf , or png .
1013+2811: pdf , or png .
J1321+2216: pdf , or png .
1311+2227: pdf , or png .
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u,v coverage for:
OJ287: pdf , or png .
J0010+1724: pdf , or png .
0210-0018: pdf , or png .
J1023+2856: pdf , or png .
0011+1446: pdf , or png .
J0216-0105: pdf , or png .
1013+2811: pdf , or png .
J1321+2216: pdf , or png .
1311+2227: pdf , or png .
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Crude maps of sources:
OJ287: pdf , or FITS .
J0010+1724: pdf , or FITS .
0210-0018: pdf , or FITS .
J1023+2856: pdf , or FITS .
0011+1446: pdf , or FITS .
J0216-0105: pdf , or FITS .
1013+2811: pdf , or FITS .
J1321+2216: pdf , or FITS .
1311+2227: pdf , or FITS .
Comments.