Add to ORKGWhy source structure affects VLBI observations and how source structure corrupts the geodetic observables are discussed. Evidence is presented which shows that corrections for source structure are possible and necessary for centimeter level accuracy VLBI measurements
The basic principles of very-long-baseline interferometry as related to its use in the determination...
The VLBI Global Observing System, which is the next generation of geodetic VLBI and is called VGOS, ...
International audienceWe present 8.4 GHz very long baseline interferometry (VLBI) observations of 48...
The celestial sources observed by geodetic very-long-baseline interferometry (VLBI), most of which a...
Errors from a number of sources in astrometric very long baseline interferometry (VLBI) have been re...
Closure quantities measured by very-long-baseline interferometry (VLBI) observations are independent...
Geodetic/astrometric very long baseline interferometry (VLBI) has been routinely observing using var...
The effects of source structure on radio interferometry measurements were investigated. The brightne...
European geodetic very long baseline interferometry (VLBI) sessions (also known as EUROPE sessions) ...
Most of the extragalactic radio sources that materialize the International Celestial Reference Frame...
The conditions for the applicability of the phase observable in very long baseline interferometry ar...
The CONT14 campaign with state-of-the-art very long baseline interferometry (VLBI) data has observed...
VLBI Global Observing System (VGOS) is now regularly observing to produce the best geodetic VLBI dat...
The next-generation, broadband geodetic very long baseline interferometry system, named VGOS, is bei...
The results of approximately 1300 observations of 67 radio sources are presented. Most of the measur...
The basic principles of very-long-baseline interferometry as related to its use in the determination...
The VLBI Global Observing System, which is the next generation of geodetic VLBI and is called VGOS, ...
International audienceWe present 8.4 GHz very long baseline interferometry (VLBI) observations of 48...
The celestial sources observed by geodetic very-long-baseline interferometry (VLBI), most of which a...
Errors from a number of sources in astrometric very long baseline interferometry (VLBI) have been re...
Closure quantities measured by very-long-baseline interferometry (VLBI) observations are independent...
Geodetic/astrometric very long baseline interferometry (VLBI) has been routinely observing using var...
The effects of source structure on radio interferometry measurements were investigated. The brightne...
European geodetic very long baseline interferometry (VLBI) sessions (also known as EUROPE sessions) ...
Most of the extragalactic radio sources that materialize the International Celestial Reference Frame...
The conditions for the applicability of the phase observable in very long baseline interferometry ar...
The CONT14 campaign with state-of-the-art very long baseline interferometry (VLBI) data has observed...
VLBI Global Observing System (VGOS) is now regularly observing to produce the best geodetic VLBI dat...
The next-generation, broadband geodetic very long baseline interferometry system, named VGOS, is bei...
The results of approximately 1300 observations of 67 radio sources are presented. Most of the measur...
The basic principles of very-long-baseline interferometry as related to its use in the determination...
The VLBI Global Observing System, which is the next generation of geodetic VLBI and is called VGOS, ...
International audienceWe present 8.4 GHz very long baseline interferometry (VLBI) observations of 48...