Galactocentric acceleration in VLBI analysis

@article{MacMillan2019GalactocentricAI,
  title={Galactocentric acceleration in VLBI analysis},
  author={D. S. MacMillan and A. L. Fey and John Gipson and David Gordon and Christopher S. Jacobs and Hana Kr{\'a}sn{\'a} and S{\'e}bastien Lambert and Zinovy Malkin and O. Titov and Guizhen Wang and M. H. Xu},
  journal={Astronomy \& Astrophysics},
  year={2019}
}
Aims. The IVS Working Group on Galactic Aberration (WG8) was established to investigate issues related to incorporating the effect of Galactic aberration in IVS analysis. The circular motion of the solar system barycenter around the Galactic center causes a change in aberration, which in the case of geodetic VLBI observing is over time scales of several decades. One of the specific goals was to recommend a Galactic aberration model to be applied by the IAU ICRF3 working group in the generation… 

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