EVN User Experiment Pipeline Feedback
Pipeline feedback for experiment ED018C_2.
If you have any comments on this experiment please email
the
address below.
A detailed
description of the pipeline output is available.
Last updated: Thu Feb 12 15:53:05 CET 2004
biggs@jive.nl
|
General Comments.
(
Brief data summary
and
scan listing
)
This is an EVN-only spectral-line experiment at 5cm (dual polarisation, 2 IFs). Participating stations were Ef, Jb (Mark2), Cm, Mc, On, Tr and Ar. No fringes were detected from Mc. The reference antenna for calibration and plotting was Ef. The EVN reliability indicator was ERI=0.53 (Ef=1.0, Jb=0.75, Cm=1.0, Mc=0.00, On=1.0, Tr=1.0, Ar=0.5) in this experiment. ERI gives you an estimate of the ratio of observed/good visibilities to the expected number visibilities. ERI* is the same but excludes data lost due to circumstances out of the EVN's control e.g. bad weather (ERI*=0.53).
Plots of the autocorrelations
.
Comments.
Cm, Tr: RFI.
Ar: No data in IF1.
Plots of the uncalibrated amplitude and phase against time
.
Comments.
Jb: no fringes in IF2, LCP.
Plots of the uncalibrated amplitude and phase against frequency
channel
.
Comments.
Cm: data seem very noisy
The uncalibrated amplitude and phase of the crosshand
correlations against frequency channel
(not available)
.
Comments.
n/a.
TSYS against time
.
Comments.
No Tsys for Cm or Ar.
Infrequent Tsys for Jb.
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.
Cm, Ar: no Tsys and so nominal gain value is used.
Jb: gain values are nonsense, much, much higher than expected from EVN status table.
Fringe-fit phase solutions
(including Parallactic Angle correction).
Comments.
None.
Fringe-fit delay solutions
.
Comments.
Solutions are very noisy. Note that scale is in microseconds.
Fringe-fit rate solutions
.
Comments.
Rates are reasonable.
Telescope bandpasses
.
Comments.
None.
Calibrated amplitude and phase against time
(a priori amplitude calibration and fringe-fit solutions applied).
Comments.
Fringe-fit has been mostly successful in calibrating the phases.
Calibrated amplitude and phase against frequency channel
.
Comments.
Bandpass is overcorrecting at high channel numbers.
Naturally weighted dirty map produced before self-cal of:
3C395
.
J2023+3153
.
Comments.
None.
Uniformly weighted dirty map produced before self-cal of:
3C395
.
J2023+3153
.
Comments.
None.
Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C395.
J2023+3153.
Comments.
None.
Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C395:
postscript
, or
text file
.
J2023+3153:
postscript
, or
text file
.
Comments.
Jb: solutions are much less than unity, as expected.
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.
Jb: sensitivity now much closer to nominal value.
Residual closure phase (visibility closure phase with model closure phase subtracted) for:
3C395
.
J2023+3153
.
Comments.
None.
Calibrated visibilities and the source model of:
3C395
.
J2023+3153
.
Comments.
None.
Calibrated visibilities against u,v distance for:
3C395.
postscript
, or
png (smaller)
J2023+3153.
postscript
, or
png (smaller)
Comments.
None.
u,v coverage for:
3C395.
postscript
, or
png (smaller)
J2023+3153.
postscript
, or
png (smaller)
Comments.
Short duration of experiment renders uv coverage poor for all sources.
Crude map of 3C395 from the pipeline
.
Crude map of J2023+3153 from the pipeline
.
Comments.
Maps are of limited quality.