| U.S. Naval Observatory | Astrometry Department |
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IVS Special Analysis Center
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The Analysis Center for Source Structure is supported and operated by the United States Naval Observatory (USNO). The main mission of the Analysis Center is to analyze VLBI data to extract intrinsic source structure information for use in maintaining the International Celestial Reference Frame (ICRF). Source structure information is provided in the form of synthesis images and source models suitable for evaluating sources for astrometric and/or geodetic use and for long-term monitoring of sources. Research into the effects of source structure on astrometric position determination is also carried out with emphasis on improving the long-term stability of the ICRF. The web server for the Analysis Center is provided by the USNO. |
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Our primary product is the Radio Reference Frame Image Database which holds information on the radio frequency intrinsic structure of most ICRF sources with declination greater than -30 degrees. Both the raw data and processed images (with their associated source models) can be obtained from this site.
Dr. Roopesh Ojha, Dr. Ralph A. Gaume, & Dr. Kerry A. Kingham |
Relevant Publications
- 2008 Annual Report (pdf)
- 2007 Annual Report (pdf)
- 2006 Annual Report (pdf)
- 2005 Annual Report (pdf)
- VLBI Observations of Southern Hemisphere ICRF Sources. II. Astrometric Suitability Based on Intrinsic Structure,"
Astronomical Journal, December 2005 issue (Vol. 130, Pages 2529-2540).- 2004 Annual Report (pdf)
- VLBI Observations of Southern Hemisphere ICRF Sources - I,"
Astronomical Journal, June 2004 issue (Vol. 127, Pages 3609-3621).- 2003 Annual Report (pdf)
- 2002 Annual Report (pdf)
- Structure Corrections in Modeling VLBI Delays for RDV Data
- AGN Variability from the USNO Radio Reference Frame Image Database
- 2001 Annual Report (pdf)
- Extragalactic Radio Source Selection for Use in Directly Linking Optical Astrometric Observations to the Radio Reference Frame
- 2000 Annual Report (pdf)
- VLBA Observations of Radio Reference Frame Sources. III. Astrometric Suitability of an Additional 225 Sources
- Geodetic VLBI Observations of EGRET Blazars
- VLBA Observations of Radio Reference Frame Sources. II. Astrometric Suitability Based on Observed Structure
- The Proper Motion of 4C 39.25
- VLBA Observations of Radio Reference Frame Sources. I.
| Last modified: Tue Dec 29 09:32:28 EST 2009 | Send comments to afey@usno.navy.mil. |