EVN User Experiment Pipeline Feedback
Last updated: Wed Feb 15 15:13:07 CET 2006
soria@jive.nl
General Comments.
(
Brief data summary
and
scan listing
)
K-band Network Monitoring Experiment observed on the 26 October 2005 session 3/2005). The experiment was recorded at 256 Mbps using 2-bit sampling, dual polarization and 8 MHz bandwidth with 16 spectral channels. Six sources were observed: 1253-055, 1611+343, CEPA and the sources 3C345 and NRAO512 in phase referencing mode, which have been pipelined.
The EVN reliability indicator (ERI) for this experiment was
ERI = 0.36 . ERI* = 0.47 .
(SH=0, EF=1, MC=1, JB=0.75, ON=1, NT=0, MH=1, UR=0.9)
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
.
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.