EVN User Experiment Pipeline Feedback


Pipeline feedback for experiment GD021B. 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 Nov 15 18:21:00 CET 2006 harvey@jive.nl

General Comments. ( Brief data summary and scan listing )
C band phase-referencing global experiment, observed on 17th June 2006. Data rate was 256 Mbps (8 X 16 MHz subbands, dual polarization, two-bit sampling). The target source 'ARP220' were calibrated using the phase-reference source '1532+234'. '1516+193', '1613+341' were also observed as calibrators.
9 stations participated. See experiment feedback for recording problems.

The EVN reliability indicator (ERI) for this experiment was ERI = 0.98 . ERI* = 0.98 . (NT=0.99, AR=1, ON=0.99, TR=0.99, WB=0.99, EF=0.93, MC=0.99, GB=1, JB=0.90)

Plots of the autocorrelations
Comments.
Noto & Torun have consistently noisy autocorrelation bandpass

plots of the uncalibrated amplitude and phase against time
Comments.

Plots of the uncalibrated amplitude and phase against frequency channel
Comments.

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

TSYS against time
Comments.

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).
Comments.

Fringe-fit phase solutions (including Parallactic Angle correction).
Comments.

Fringe-fit delay solutions
Comments.

Fringe-fit rate solutions
Comments.

Telescope bandpasses
Comments.
Gb IF4 (LL) drops off towards edge of band

Calibrated amplitude and phase against time (a priori amplitude calibration and fringe-fit solutions applied).
Comments.

Calibrated amplitude and phase against frequency channel
Comments.

Naturally weighted dirty map (not useful for bright sources) produced before self-cal of:
: pdf (not available) , or FITS (not available) .
Comments.

Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
: pdf (not available) , or FITS (not available) .
Comments.

Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
(not available) .
Comments.

Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
: pdf (not available) , or text file (not available) , or statistical summary (not available) .
Comments.

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).
Comments.

Residual closure phase (visibility closure phase with model closure phase subtracted) for:
(not available) .
Comments.

Calibrated visibilities and the source model of:
(not available) .
Comments.

Calibrated visibilities against u,v distance for:
: pdf (not available) , or png (not available) .
Comments.

u,v coverage for:
: pdf (not available) , or png (not available) .
Comments.

Crude maps of sources:
: pdf (not available) , or FITS (not available) .
Comments.