The Gaia reference frame for bright sources examined using VLBI observations of radio stars ( Corrigendum)

摘要

This is a corrigendum to Lindegren (2020). Owing to a codingerror in the implementation of the analysis method described inthe paper, the results obtained from its application to Gaia DR2data were significantly wrong. Although the main conclusionsof the original paper remain unchanged, the results presentedin Tables 2 and 3, Figs. 3–5, and Sects. 3.3, 3.4, 4, and 5 aresubstantially affected. The revised tables, figures, and portionsof the text are given below.