VLBI global solution 2005f_astro
Astrometric global solution 2005f_astro used all available VLBI observations
including 21 observing sessions of the
VLBA Calibrator Survey
at 8.6GHz and 2.2 GHz from 1979.08.03 to 2005.12.01, 4059 twenty four hour
sessions, 5.14 millions measurements of group delays.
Positions of 3481 sources were adjusted in a single least square solution.
Currently, this is the most complete catalogue of positions of compact
radio sources. Technical description of the solution is available
here.
Astrometric Results
-
2005f_astro catalogue in
HTML form (7.3 Mb). NB: loading the catalogue
takes time, please be patient. The catalogue contains source
positions, their uncertainties, estimates of the total VLBA flux
density, the VLBA flux density of unresolved components, naturally
weighted CLEAN images in postscript and in fits format at X and
S-band; plots of the correlated flux density as a function of the
length of the baseline projection to the source plane; fits files
with calibrated uv data. So far images and fluxes are
available only for 1414 sources.
-
2005f_astro catalogue in ASCII format.
The catalogue contains source positions, their uncertainties,
total VLBA flux density, the VLBA flux density of unresolved
components.
-
2005f_astro catalogue in key-format
format. The catalogue contains source positions.
This catalogue can be used as a priori file for
VLBI SCHED
scheduling software package.
-
2005f_astro catalogue in blokq
format. The catalogue contains source positions and
their uncertainties. This catalogue can be used as a priori
file for Mark5 VLBI
analysis software package Calc/Solve.
-
Images and calibrated uv data of 1414
sources in one tar.bz2 file (2127Mb).
Refer to readme file
for the file name convention in this archive. NB: the size of
this file is greater than 2Gb. Your broweser probably will not be able
to download it. It is suggested to use
wget-1.10
or newer for downloading this file.
- Interactive
calibrators search tool among sources in the 2005f_astro
catalogue.
Geophysics Results
Station positions and velocities
Positions of 151 stations and their velocities were estimated as global
parameters. Station positions are given on epoch 1997.01.01
Earth orientation parameters
Pole coordinates X, Y, UT1 angle, and their rate, daily correction to the
nutation in longitude and nutation in obliquity were estimated for each
session separately.
Assessment of accuracy of EOP series
Comparison of EOP parameters determined from 80 simultaneous 24 hours
VLBI experiments at networks CORE-A and NEOS-A.
- Plot of differences in
X pole coordinates;
- Plot of differences in
Y pole coordinates;
- Plot of differences in
UT1 angles;
- Plot of differences in
nutation in longitude;
- Plot of differences in
nutation in obliquity;
- Plot of differences in
X pole rates;
- Plot of differences in
Y pole rates;
- Plot of differences in
UT1 rates;
- Table of statistics of the
differences.
Statistics
Comparison of EOP series
Comparison with
IERS C04
series shows random noise with slight linear trend with scatter comparable
with the accuracy of VLBI EOP series, except UT1 where the noise of IERS C04
series is dominating.
- Plot of the differences with IERS C04 in
X pole coordinates;
- Plot of the differences with IERS C04 in
Y pole coordinates;
- Plot of the differences with IERS C04 in
UT1 angles;
- Table of statistics of the
differences.
Miscellaneous
Usage policy: you can download files for research purposes, you can put links
to this Web page, but you cannot post any part of content of this Web
page on ftp or http servers without prior written permission from authors.
Back to
Goddard VLBI astrometric catalogues .
Web page was prepared by Leonid Petrov
(
)
Last update: 2005.12.21_05:09:07