Astrometry

The AllWISE Catalog as an Infrared Celestial Reference Frame in the Gaia Era
AllWISE 与 Gaia DR3参考架系统偏差好于 5 mas、相对旋转小于 0.1 mas yr⁻¹，可作为高精度红外天球参考架。
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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
中国空间站工程巡天望远镜（CSST）的天体测量精度估计
We estimated the astrometric performance of the China Space Station Telescope Sky Survey in extending the Gaia Celestial Reference Frame by using a simulated set of sources.
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中国空间站工程巡天望远镜（CSST）的天体测量精度估计
Systematics of planetary ephemeris reference frames inferred from pulsar timing astrometry
基于脉冲星计时观测比较行星历表参考架，结果显示其定向精度优于0.4毫角秒，非惯性旋转优于5微角秒每年。
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Systematics of planetary ephemeris reference frames inferred from pulsar timing astrometry
基于计时、Gaia 与射电干涉测量的脉冲星位置比较：动力学与运动学参考架的对比
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书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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基于计时、Gaia 与射电干涉测量的脉冲星位置比较：动力学与运动学参考架的对比
Effect of Galactic aberration on Earth orientation parameters: From the ICRF2 to the ICRF3
We estimated the effect of Galactic aberration on Earth orientation parameters based on geodetic/astrometric very long baseline interferometry data.
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Effect of Galactic aberration on Earth orientation parameters: From the ICRF2 to the ICRF3