International audienceThis paper reports on the detection of the Galactic aberration in astrometric measurements of quasar positions by very long baseline radio interferometry (VLBI). The Galactic aberration effect shows up as a dipole component in the quasar proper motion field, oriented towards the Galactic center. The dipole amplitude is in good agreement with theoretical predictions
International audienceMost of the radio sources observed by VLBI, some used as defining sources in t...
Most of the radio sources observed by VLBI, some used as defining sources in the International Celes...
Abstract—The influence of proper motions of sources due to Galactic aberration on precession models ...
International audienceThis paper reports on the detection of the Galactic aberration in astrometric ...
International audienceThis paper reports on the detection of the Galactic aberration in astrometric ...
International audience Aims: While analyzing decades of very long baseline interferometry (VLBI) dat...
International audience Aims: While analyzing decades of very long baseline interferometry (VLBI) dat...
International audience Aims: While analyzing decades of very long baseline interferometry (VLBI) dat...
International audienceThe IVS Working Group on Galactic Aberration (WG8) was established to investig...
International audienceThe IVS Working Group on Galactic Aberration (WG8) was established to investig...
Aims. While analyzing decades of very long baseline interferometry (VLBI) data, we detecte...
International audienceAnalysis of VLBI records of distant radio source signals allows to determine t...
International audienceAnalysis of VLBI records of distant radio source signals allows to determine t...
International audienceAnalysis of VLBI records of distant radio source signals allows to determine t...
International audienceMost of the radio sources observed by VLBI, some used as defining sources in t...
International audienceMost of the radio sources observed by VLBI, some used as defining sources in t...
Most of the radio sources observed by VLBI, some used as defining sources in the International Celes...
Abstract—The influence of proper motions of sources due to Galactic aberration on precession models ...
International audienceThis paper reports on the detection of the Galactic aberration in astrometric ...
International audienceThis paper reports on the detection of the Galactic aberration in astrometric ...
International audience Aims: While analyzing decades of very long baseline interferometry (VLBI) dat...
International audience Aims: While analyzing decades of very long baseline interferometry (VLBI) dat...
International audience Aims: While analyzing decades of very long baseline interferometry (VLBI) dat...
International audienceThe IVS Working Group on Galactic Aberration (WG8) was established to investig...
International audienceThe IVS Working Group on Galactic Aberration (WG8) was established to investig...
Aims. While analyzing decades of very long baseline interferometry (VLBI) data, we detecte...
International audienceAnalysis of VLBI records of distant radio source signals allows to determine t...
International audienceAnalysis of VLBI records of distant radio source signals allows to determine t...
International audienceAnalysis of VLBI records of distant radio source signals allows to determine t...
International audienceMost of the radio sources observed by VLBI, some used as defining sources in t...
International audienceMost of the radio sources observed by VLBI, some used as defining sources in t...
Most of the radio sources observed by VLBI, some used as defining sources in the International Celes...
Abstract—The influence of proper motions of sources due to Galactic aberration on precession models ...