 VLBI global solution rfc_2012b
 VLBI global solution rfc_2012b 
   Astrometric global solution rfc_2012b used all available VLBI observations
at 8.6GHz and 2.2 GHz, as well at 5 and 22GHz from 1980.04.11 through
2012.04.02, in total 5381 observing sessions, including 329 observing
sessions dedicated to the absolute astrometry surveys,
such as
  -  24 observing sessions of VLBA Calibrator Survey;
       
 
-  9 observing sessions of the Australian LBA Calibrator Survey;
       
 
-  85 observing sessions of the   VLBI 2MASS radioastronomy project;
       
 
-  16 observing sessions of the 
       VLBA Imaging and Polarimetry Survey (VIPS);
       
 
-  132 regular geodetic VLBA sessions under the RDV program;
       
 
-  3 observing sessions in 1FGL AGNs at parsec scales;
       
 
-  3 observing sessions of VLBA Galactic Plan Survey;
       
 
-  1 observing session of the EVN  Galactic Plan Survey
       at K-band;
       
 
-  14 observing sessions of the K/Q survey;
       
 
-  34 observing sessions of the VLBA calibrator survey for BeSSeL
       project;
       
 
-  2 observing sessions of the Bologna survey of near galaxies;
       
 
-  3 observing sessions of the VLBA survey of flat-Spectrum FIRST Sources;
       
 
-  3 observing sessions of the CJ snap-shot survey with the VLBA;
       
 
-  3 EVN observing sessions for densification of the ICRF
       
 
-  7 observing session of the survey of optically bright quasars;
       
 
-  2 observing sessions of the compactness of weak radio sources at
       high frequency survey 
 
In total,  9521432  estimates of group delays were used in
LSQ solutions.
Positions of 7049 sources were adjusted in 5 least square solutions
for X/S, X-band, S-band, C-band, and K-band solutions. Currently, this
is the most complete catalogue of positions of compact radio sources.
Technical description of the solution is available
here.
 Astrometric Results 
  -  
       rfc_2012b catalogue in
       HTML form (10 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. Images and estimates of
       correlated flux densities are available for 3714 sources from this
       catalogue. Among 7049 sources, 5868 are classified as calibrators,
       1082 are classified as non-calibrators with reliable positions and
       100 are classified as non-calibrators with unreliable positions.
       For the sources from the latter class, there is a probability > 0.001
       that group delay ambiguities were resolved incorrectly, and as a result,
       their position may be off in a range of 0."1 to 5' from the reported
       coordinates.
       
  
-  
       rfc_2012b  catalogue in ASCII format.
       The catalogue contains source positions, their uncertainties,
       total VLBA flux density, the VLBA flux density of unresolved
       components.
       
  
-  
       rfc_2012b  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.
       
  
-  
       rfc_2012b  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.
       
  
-  Interactive
       VLBI calibrator search tool among sources in the rfc_2012b
       catalogue.
       
 Astrophysics Information 
  -  
       28,853 Images and calibrated uv data
        for  4321  sources at
       S, C, X, U, K, Q, and W bands in one tar.bz2 file (33 Gb).
       For some of the sources images for more than one epoch are available.
       
-  
       Single dish spectrum
        for  6791  sources from
       published results determined with use of the CATS database.
       NB: the estimates of flux density are NOT simultaneous. Since
       the majority of sources are variable, these estimates of the spectrum
       are not always reliable. Estimates of spectrum for some sources
       may be wrong due to errors in the database of singe dish flux
       measurements.
       
 Geophysics Results 
 Station positions and velocities 
     Positions of 170 stations and their velocities were estimated as global
     parameters. Station positions are given on epoch 2000.01.01.
     Boundary conditions were selected in such a way that source positions,
     station positions and velocities are compatible with USNO series of the
     Earth orientation parameters
     finals.all and
     finals.daily.
     
 Antenna axis offsets 
Antenna axis offsets from LSQ estimation    
  rfc_2012b.axof
 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.
     
 Statistics 
     
 Miscellaneous 
     
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Back to Astrogeo Center home page. 
    Web page was prepared by Leonid Petrov
    ( )
) 
   
   Last update: 2012.06.17_05:29:03