EVN User Experiment Pipeline Feedback
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.