ICRF3

Evaluate the ICRF3 Axes' Stability via Extragalactic Source Position Time Series
VLBI source position time series indicate that the ICRF3 axes are stable at the 10–20 microarcsecond level and confirm the robustness of the commonly used four-step solution.
PDF Cite Code Dataset arXiv Proceedings
Evaluate the ICRF3 Axes' Stability via Extragalactic Source Position Time Series
Is there an interest in bringing Gaia-CRF into VLBI data reduction?
An exploratory study of using Gaia-CRF2 in VLBI data reduction examines how celestial-frame constraints affect source positions, Earth orientation parameters, and the terrestrial reference frame.
PDF Cite ADS
Is there an interest in bringing Gaia-CRF into VLBI data reduction?