Gaia

Astrometric Systematic Errors as a Limiting Factor in Stellar-Aberration-Based Autonomous Navigation
通过九种底片常数模型的全天评估，表明底片常数解误差对恒星光行差自主导航将产生米每秒量级的速度误差贡献。
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Astrometric Systematic Errors as a Limiting Factor in Stellar-Aberration-Based Autonomous Navigation
Astrometric properties of reference frame sources as a function of redshift
基于 RFC 与 Gaia 数据，揭示光学天体测量性质及射电—光学位置偏移的红移变化趋势主要与星等和源群体差异有关，而 VLBI 性质未显示显著的红移依赖。
PDF 引用 DOI arXiv
Astrometric properties of reference frame sources as a function of redshift
An infrared celestial reference frame realized by the CatWISE2020 catalog
通过与Gaia DR3交叉匹配，研究CatWISE2020的位置和自行系统误差，表明其在完成系统误差改正后可作为国际天球参考系在红外波段的一种实现。
引用 DOI
An infrared celestial reference frame realized by the CatWISE2020 catalog
Statistical analysis of quasars in LQAC-6: astrometry, brightness, and redshift
对LQAC-6中200余万个类星体的天区分布、天体测量不确定度、红移一致性和光学光度开展统计分析，为天球参考架源的选择与评估提供依据。
引用 数据集 DOI
Statistical analysis of quasars in LQAC-6: astrometry, brightness, and redshift
Comparison of the Gaia-CRF3 and planetary ephemerides via asteroid observations
利用 Gaia 小行星观测比较 Gaia-CRF3 与 DE440 动力学参考架；仅用传统观测时偏差约 10 mas，加入 Gaia 数据后降至 0.2 mas。
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Comparison of the Gaia-CRF3 and planetary ephemerides via asteroid observations
The AllWISE Catalog as an Infrared Celestial Reference Frame in the Gaia Era
通过与 Gaia DR3 比较，评估 AllWISE 的天体测量特性及其作为红外天球参考架的应用。
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The AllWISE Catalog as an Infrared Celestial Reference Frame in the Gaia Era
Secular aberration drift in stellar proper motions. An additional term due to the change in line-of-sight direction
本文发现长期光行差漂移中存在一个由视线方向变化引起的附加项，对 Gaia 观测的恒星自行产生可测量影响。
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Secular aberration drift in stellar proper motions. An additional term due to the change in line-of-sight direction
The Astrometric Performance of the China Space Station Telescope (CSST) Sky Survey in Extending the Gaia Celestial Reference Frame
通过模拟观测，评估 CSST 巡天拓展 Gaia 天球参考架的精度与潜力。
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The Astrometric Performance of the China Space Station Telescope (CSST) Sky Survey in Extending the Gaia Celestial Reference Frame
Comparison of dynamical and kinematic reference frames via pulsar positions from timing, Gaia, and interferometric astrometry
本文利用脉冲星由计时、VLBI 与 Gaia 独立测得的位置，在亚毫角秒精度上评估行星历表所代表的动力学参考架与 Gaia/VLBI 所实现的运动学参考架之间的定向一致性。
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Comparison of dynamical and kinematic reference frames via pulsar positions from timing, Gaia, and interferometric astrometry
Comparison of multifrequency positions of extragalactic sources from ICRF3 and Gaia EDR3
比较 ICRF3 与 Gaia EDR3 的源位置，分析射电源结构对射电—光学位置偏移的影响。
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Comparison of multifrequency positions of extragalactic sources from ICRF3 and Gaia EDR3