We report on recent VLBA/VERA/IVS observational tests of General Relativity. First, we will summarize the results from the 2005 VLBA experiment that determined gamma with an accuracy of 0.0003 by measuring the deflection of four compact radio sources by the solar gravitational field. We discuss the limits of precision that can be obtained with VLBA experiments in the future. We describe recent experiments using the three global arrays to measure the aberration of gravity when Jupiter and Saturn passed within a few arcmin of bright radio sources. These reductions are still in progress, but the anticipated positional accuracy of the VLBA experiment may be about 0.01 mas.Sergei Kopeikin thanks the Research Council (Grant No. C1669103) and Alum...
International audienceThe original VLBA Calibrator Surveys (VCS) were a series of 6 VLBA campaigns f...
International audienceRelativistic bending in the vicinity of a massive body is characterized only b...
The Japanese lunar explorer SELENE (KAGUYA), which has been launched on Sep. 14th, 2007, utilizes VL...
Since VLBI techniques give microarcsecond position accuracy of celestial objects, tests of GR using ...
We have used the Very Long Baseline Array (VLBA) at 43, 23, and 15 GHz to measure the solar gravitat...
Context. We highlight the capabilities of geodetic VLBI technique to test general relativity in the ...
Context: We highlight the capabilities of geodetic VLBI technique to test general relativity in the ...
We have determined the relativistic light deflection of the quasar J0842+1835 as Jupiter passed with...
General relativity (GR) predicts that photons are delayed and deflected by the space curvature produ...
International audience Aims: This study revisits the estimate of the post-Newtonian relativistic par...
International audienceAims: Relativistic bending in the vicinity of a massive body is characterized ...
According to general relativity, photons are deflected and delayed by the curvature of space-time pr...
International audience Aims: While analyzing decades of very long baseline interferometry (VLBI) dat...
Once the afterglow from a GRB has been detected in the radio, Very Long Baseline Interferometry (VLB...
International audienceThe original VLBA Calibrator Surveys (VCS) were a series of 6 VLBA campaigns f...
International audienceRelativistic bending in the vicinity of a massive body is characterized only b...
The Japanese lunar explorer SELENE (KAGUYA), which has been launched on Sep. 14th, 2007, utilizes VL...
Since VLBI techniques give microarcsecond position accuracy of celestial objects, tests of GR using ...
We have used the Very Long Baseline Array (VLBA) at 43, 23, and 15 GHz to measure the solar gravitat...
Context. We highlight the capabilities of geodetic VLBI technique to test general relativity in the ...
Context: We highlight the capabilities of geodetic VLBI technique to test general relativity in the ...
We have determined the relativistic light deflection of the quasar J0842+1835 as Jupiter passed with...
General relativity (GR) predicts that photons are delayed and deflected by the space curvature produ...
International audience Aims: This study revisits the estimate of the post-Newtonian relativistic par...
International audienceAims: Relativistic bending in the vicinity of a massive body is characterized ...
According to general relativity, photons are deflected and delayed by the curvature of space-time pr...
International audience Aims: While analyzing decades of very long baseline interferometry (VLBI) dat...
Once the afterglow from a GRB has been detected in the radio, Very Long Baseline Interferometry (VLB...
International audienceThe original VLBA Calibrator Surveys (VCS) were a series of 6 VLBA campaigns f...
International audienceRelativistic bending in the vicinity of a massive body is characterized only b...
The Japanese lunar explorer SELENE (KAGUYA), which has been launched on Sep. 14th, 2007, utilizes VL...