EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment GJ010A. 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 Jun 30 14:54:16 CEST 2004 biggs@jive.nl

General Comments. (Brief data summary (not available) and scan listing (not available) )

Plots of the autocorrelations (not available) .
Comments.

Plots of the uncalibrated amplitude and phase against time (not available) .
Comments.

Plots of the uncalibrated amplitude and phase against frequency channel (not available) .
Comments.

The uncalibrated amplitude and phase of the crosshand correlations against frequency channel (not available) .
Comments.

TSYS against time (not available) .
Comments.

Telescope sensitivities (not available) from the a priori TSYS and Gain curves (the square of this number gives the antenna noise (SEFD) in Jy - the smaller the better).
Comments.

Fringe-fit phase solutions (not available) (including Parallactic Angle correction).
Comments.

Fringe-fit delay solutions (not available) .
Comments.

Fringe-fit rate solutions (not available) .
Comments.

Telescope bandpasses (not available) .
Comments.

Calibrated amplitude and phase against time (not available) (a priori amplitude calibration and fringe-fit solutions applied).
Comments.

Calibrated amplitude and phase against frequency channel (not available) .
Comments.

Naturally weighted dirty map produced before self-cal of:
0552+398:postscript (not available) , or FITS (not available) .
2007+777:postscript (not available) , or FITS (not available) .
P2319:postscript (not available) , or FITS (not available) .
Comments.

Uniformly weighted dirty map produced before self-cal of:
0552+398:postscript (not available) , or FITS (not available) .
2007+777:postscript (not available) , or FITS (not available) .
P2319:postscript (not available) , or FITS (not available) .
Comments.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
0552+398. (not available)
2007+777. (not available)
P2319. (not available)
Comments.

Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
0552+398: postscript (not available) , or text file (not available) .
2007+777: postscript (not available) , or text file (not available) .
P2319: postscript (not available) , or text file (not available) .
Comments.

Telescope sensitivities (not available) (the total AMP gain applied during both a priori and self calibration; the square of this number gives the antenna noise (SEFD) in Jy).
Comments.

Residual closure phase (visibility closure phase with model closure phase subtracted) for:
0552+398 (not available) .
2007+777 (not available) .
P2319 (not available) .
Comments.

Calibrated visibilities and the source model of:
0552+398 (not available) .
2007+777 (not available) .
P2319 (not available) .
Comments.

Calibrated visibilities against u,v distance for:
0552+398. postscript (not available) , or png (smaller) (not available)
2007+777. postscript (not available) , or png (smaller) (not available)
P2319. postscript (not available) , or png (smaller) (not available)
Comments.

u,v coverage for:
0552+398. postscript (not available) , or png (smaller) (not available)
2007+777. postscript (not available) , or png (smaller) (not available)
P2319. postscript (not available) , or png (smaller) (not available)
Comments.

0552+398:postscript (not available) , or FITS (not available) .
2007+777:postscript (not available) , or FITS (not available) .
P2319:postscript (not available) , or FITS (not available) .
Comments.