VLBI global solution rfc_2015d

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The contents of this web page and following links contains unpublished material. The material is provided as a courtesy for the preview. Using this material in publications, copying, and posting on Internet is not allowed without written prior permission.

Astrometric global solution rfc_2015d used all available VLBI observations at 8.6GHz and 2.2 GHz, as well at 5 and 22GHz from 1980.04.11 through 2015.09.24, in total 6124 observing sessions, including 445 observing sessions dedicated to the absolute astrometry surveys, such as

• 24 observing sessions of VLBA Calibrator Survey;
  
• 17 observing sessions of Densification of the VLBA Calibrator Survey (VCS7);
  
• 10 observing sessions of Densification of the VLBA Calibrator Survey (VCS8);
  
• 6 observing sessions of Densification of the VLBA Calibrator Survey (VCS9);
  
• 16 observing sessions of the Australian LBA Calibrator Survey;
  
• 94 observing sessions of the VLBI 2MASS radioastronomy project;
  
• 16 observing sessions of the VLBA Imaging and Polarimetry Survey (VIPS);
  
• 145 regular geodetic VLBA sessions under the RDV program;
  
• 13 observing sessions in 1FGL, 2FGL, and 3FGL 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 VLBA+EVN observing session of the survey of optically bright quasars;
  
• 11 VLBA observing session of the survey for parallax measurements;
  
• 17 VLBA observing session of gamma-ray follow-up
  
• 2 observing sessions of the compactness of weak radio sources at high frequency survey
  
• 5 observing sessions of the VLBI Ecliptic Plane Survey at the CVN
  

Positions of 9763 sources were adjusted in 6 least square solutions for X/S, X/C, 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

1. rfc_2015d catalogue in HTML form (24 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 7265 sources from this catalogue. Among 9763 sources, 6098 are classified as calibrators, 3476 are classified as non-calibrators with reliable positions and 189 are classified as non-calibrators with unreliable positions.
2. rfc_2015d catalogue in ASCII format. The catalogue contains source positions, their uncertainties, total VLBA flux density, the VLBA flux density of unresolved components.
3. rfc_2015d 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.
4. rfc_2015d catalogue in blokq format. The catalogue contains source positions and their uncertainties. This catalogue can be used as a priori file for library and Mark5 VLBI analysis software package Calc/Solve.
5. Interactive VLBI calibrator search tool among sources in the rfc_2015d catalogue.

Astrophysics Information

1. 40,068 Images and calibrated uv data for 7265 sources at S, C, X, U, K, Q, and W bands in one tar.bz2 file (58 Gb). For some of the sources images for more than one epoch are available.
2. Single dish spectrum for 9176 sources from published results determined with the 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

Station positions catalogue from XS observations		Format description
Station positions catalogue from X-band only observations		Format description
Station positions catalogue from C-band only observations		Format description
Station positions catalogue from K-band only observations		Format description
Station velocity catalogue		Format description
Empirical model of aharmonic non-linear site motion		Format description
Empirical model of harmonic site motion		Format description

Antenna axis offsets

Earth orientation parameters

EOP time series in Solve EOB format		Format description
EOP time series in Solve NUT format		Format description
EOP time series in IVS format		Format description
Correlations between EOP estimates		Format description

Statistics

Miscellaneous

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Web page was prepared by Leonid Petrov ()
Last update: 2015.11.08_02:06:34