EVN User Experiment Pipeline Feedback
Last updated: Thu Feb 16 14:43:21 CET 2006
harvey@jive.nl
General Comments.
(
Brief data summary
and
scan listing
)
Wb had major problems with the 1Gbps recording in this session, which left the target sources with less time producing good data for this station. We have now fixed this problem for future observing runs.Mc also didn't have enough bandwidth to handle the full 1Gbps observations and experienced RFI.
The EVN reliability indicator (ERI) for this experiment was
ERI = 0.845 . ERI* = 0.845 .
(WB=0.675, MC=0.75, UR=0.85, EF=0.81, SH=0.83, JB=1, TR=1)
Plots of the autocorrelations
.
Comments.
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.
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:
:postscript
(not available)
, or
FITS
(not available)
.
Comments.
Uniformly weighted dirty map (not useful for bright sources) produced before self-cal of:
:postscript
(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.
: postscript (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:
. postscript (not available)
, or png (smaller)
(not available)
Comments.
u,v coverage for:
. postscript (not available)
, or png (smaller)
(not available)
Comments.
Crude maps of sources:
:postscript
(not available)
, or
FITS
(not available)
.
Comments.