利用射电恒星的 VLBI 观测检验明亮来源的盖亚参照基准（更正）

IF 6.5 2区物理与天体物理

Astronomy & Astrophysics Pub Date : 2020-05-01 DOI:10.1051/0004-6361/201936161e

L. Lindegren

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引用次数: 2

摘要

本文是对 Lindegren (2020) 的更正。由于论文中描述的分析方法在实施过程中出现了编码错误，因此将其应用于 Gaia DR2 数据所得到的结果出现了重大错误。虽然原论文的主要结论没有改变，但表 2 和表 3、图 3-5 以及第 3.3、3.4 和 3.5 节中的结果却发生了变化。3.3、3.4、4 和 5 节中的结果受到很大影响。修订后的表、图和部分文字如下。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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

This is a corrigendum to Lindegren (2020). Owing to a coding error in the implementation of the analysis method described in the paper, the results obtained from its application to Gaia DR2 data were significantly wrong. Although the main conclusions of the original paper remain unchanged, the results presented in Tables 2 and 3, Figs. 3–5, and Sects. 3.3, 3.4, 4, and 5 are substantially affected. The revised tables, figures, and portions of the text are given below.

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来源期刊

Astronomy & Astrophysics ASTRONOMY & ASTROPHYSICS-

自引率

27.70%

发文量

期刊介绍： Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.