EVN Network Monitoring Experiment (NME) Pipeline Feedback
Last updated: Tue Sep 20 18:15:34 CEST 2005
anderson@jive.nl
General Comments.
(
Brief data summary
and
scan listing
)
N05L2 was an L-Band Network Monitoring Experiment, combined with a series of test observations for ionospheric calibration. 3C273B was observed twice for FTP fringe testing. Other bright calibrator sources were observed in a phase-referencing style mode to test ionospheric calibration techniques.
Observed on 2005 June 02
256 Mb s^{-1}, 4x8 MHz subbands, dual polarization, 0.5 s integrations, cross polarizations included
Tr, Torun: BBC\# 3 was unlocked all the time, resulting in loss of data. Used Rubidium frequency standard, because the H-maser was sent to the manufacturer for refurbishment.
EF missing from scan 1.
The EVN reliability indicator (ERI) for this experiment was
ERI = JB 0.9 WB 1 EF 1 ON 0.66 MC 1 TR 0.88 NT 1 SH 1 UR 1 CM 1 HH 1
ERI = 0.90
. ERI* = JB 0.9 WB 1 EF 1 ON 0.66 MC 1 TR 0.88 NT 1 SH 1 UR 1 CM 1 HH 1
ERI* = 0.90
.
(JB=1, ON=0.8 ...)
Plots of the autocorrelations
.
Comments.
Plots of the uncalibrated amplitude and phase against time
.
Comments.
Flagging needed
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.
JB missing TSYS values for many scans, especially 3C273B
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.
CM needs flagging on IF 4 for microwave link bandpass effects
Fringe-fit rate solutions
.
Comments.
Telescope bandpasses
.
Comments.
CM needs flagging on IF 4 for microwave link bandpass effects
Calibrated amplitude and phase against time
(a priori amplitude calibration and fringe-fit solutions applied).
Comments.
Flagging needed
Calibrated amplitude and phase against frequency channel
.
Comments.
Naturally weighted dirty map produced before self-cal of:
3C273B:
postscript
, or
FITS
.
J1159-2148:
postscript
, or
FITS
.
J1159-2228:
postscript
, or
FITS
.
J1212-2221:
postscript
, or
FITS
.
J1215-1731:
postscript
, or
FITS
.
J1218-0119:
postscript
, or
FITS
.
J1222+0413:
postscript
, or
FITS
.
J1224+0330:
postscript
, or
FITS
.
J1636+2112:
postscript
, or
FITS
.
J1641+2257:
postscript
, or
FITS
.
J1642+2523:
postscript
, or
FITS
.
J1644+1813:
postscript
, or
FITS
.
Comments.
Uniformly weighted dirty map produced before self-cal of:
3C273B:
postscript
, or
FITS
.
J1159-2148:
postscript
, or
FITS
.
J1159-2228:
postscript
, or
FITS
.
J1212-2221:
postscript
, or
FITS
.
J1215-1731:
postscript
, or
FITS
.
J1218-0119:
postscript
, or
FITS
.
J1222+0413:
postscript
, or
FITS
.
J1224+0330:
postscript
, or
FITS
.
J1636+2112:
postscript
, or
FITS
.
J1641+2257:
postscript
, or
FITS
.
J1642+2523:
postscript
, or
FITS
.
J1644+1813:
postscript
, or
FITS
.
Comments.
Phase corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C273B.
J1159-2148.
J1159-2228.
J1212-2221.
J1215-1731.
J1218-0119.
J1222+0413.
J1224+0330.
J1636+2112.
J1641+2257.
J1642+2523.
J1644+1813.
Comments.
Amplitude corrections applied to a priori calibrated and fringe-fitted data by self-calibration.
3C273B:
postscript
, or
text file
.
J1159-2148:
postscript
, or
text file
.
J1159-2228:
postscript
, or
text file
.
J1212-2221:
postscript
, or
text file
.
J1215-1731:
postscript
, or
text file
.
J1218-0119:
postscript
, or
text file
.
J1222+0413:
postscript
, or
text file
.
J1224+0330:
postscript
, or
text file
.
J1636+2112:
postscript
, or
text file
.
J1641+2257:
postscript
, or
text file
.
J1642+2523:
postscript
, or
text file
.
J1644+1813:
postscript
, or
text file
.
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.
JB, ON, NT, SH, HH missing in plot for most time until ~17:30
Residual closure phase (visibility closure phase with model closure phase subtracted) for:
3C273B
.
J1159-2148
.
J1159-2228
.
J1212-2221
.
J1215-1731
.
J1218-0119
.
J1222+0413
.
J1224+0330
.
J1636+2112
.
J1641+2257
.
J1642+2523
.
J1644+1813
.
Comments.
Calibrated visibilities and the source model of:
3C273B
.
J1159-2148
.
J1159-2228
.
J1212-2221
.
J1215-1731
.
J1218-0119
.
J1222+0413
.
J1224+0330
.
J1636+2112
.
J1641+2257
.
J1642+2523
.
J1644+1813
.
Comments.
Calibrated visibilities against u,v distance for:
3C273B.
postscript
, or
png (smaller)
J1159-2148.
postscript
, or
png (smaller)
J1159-2228.
postscript
, or
png (smaller)
J1212-2221.
postscript
, or
png (smaller)
J1215-1731.
postscript
, or
png (smaller)
J1218-0119.
postscript
, or
png (smaller)
J1222+0413.
postscript
, or
png (smaller)
J1224+0330.
postscript
, or
png (smaller)
J1636+2112.
postscript
, or
png (smaller)
J1641+2257.
postscript
, or
png (smaller)
J1642+2523.
postscript
, or
png (smaller)
J1644+1813.
postscript
, or
png (smaller)
Comments.
u,v coverage for:
3C273B.
postscript
, or
png (smaller)
J1159-2148.
postscript
, or
png (smaller)
J1159-2228.
postscript
, or
png (smaller)
J1212-2221.
postscript
, or
png (smaller)
J1215-1731.
postscript
, or
png (smaller)
J1218-0119.
postscript
, or
png (smaller)
J1222+0413.
postscript
, or
png (smaller)
J1224+0330.
postscript
, or
png (smaller)
J1636+2112.
postscript
, or
png (smaller)
J1641+2257.
postscript
, or
png (smaller)
J1642+2523.
postscript
, or
png (smaller)
J1644+1813.
postscript
, or
png (smaller)
Comments.
Crude maps of sources:
3C273B:
postscript
, or
FITS
.
J1159-2148:
postscript
, or
FITS
.
J1159-2228:
postscript
, or
FITS
.
J1212-2221:
postscript
, or
FITS
.
J1215-1731:
postscript
, or
FITS
.
J1218-0119:
postscript
, or
FITS
.
J1222+0413:
postscript
, or
FITS
.
J1224+0330:
postscript
, or
FITS
.
J1636+2112:
postscript
, or
FITS
.
J1641+2257:
postscript
, or
FITS
.
J1642+2523:
postscript
, or
FITS
.
J1644+1813:
postscript
, or
FITS
.
Comments.