collaborators

5 papers

astro-ph.GA2026

Optical-morphology-based assessment of astrometric quality in Gaia-CRF3 quasars

Qiqi Wu, Shilong Liao, Zhaoxiang Qi +3

Context. Several studies have shown that host-galaxy structure or extended optical morphology in AGNs can induce spurious parallaxes and proper motions in Gaia DR3. However, it rem…

astro-ph.IM2026

Refining the Gaia DR3 Parallax Zero-point: A Hybrid Approach Combining Global Parametric Correction with Local Refinement

Ye Ding, Shilong Liao, Zhaoxiang Qi +3

The Gaia Data Release 3 (GDR3) parallaxes are affected by a complex bias that depends on stellar magnitude, color, and celestial position, with amplitudes reaching tens of microarc…

astro-ph.IM2026

Constraining the inclination of binary system orbits with the astrometric excess noise from Gaia DR3

Shilong Liao, Ye Ding, Shangyu Wen +2

Orbital inclination is crucial in determining the binary mass. The astrometric excess noise contains the orbital motion information, which can be used to constrain the inclination.…

astro-ph.GA2025

Characterizing the astrometric quality of AGNs in Gaia-CRF3

Shilong Liao, Qiqi Wu, Ye Ding +2

Active Galactic Nuclei (AGNs), owing to their great distances and compact sizes, serve as fundamental anchors for defining the celestial reference frame. With about 1.9 million AGN…

astro-ph.SR2025

Analysis of the Gaia Data Release 3 parallax bias at bright magnitudes

Ye Ding, Shilong Liao, Shangyu Wen +1

The combination of visual and spectroscopic orbits in binary systems enables precise distance measurements without additional assumptions, making them ideal for examining the paral…