collaborators

6 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.IM2026

A Gaia-linked High-purity QSO Candidate Catalog in Selected Fields with Extinction-binned Calibration and Spectrum-informed Training

Zi-Huang Cao, Zhao-Xiang Qi, Juan-Juan Ren +11

We present an extinction-calibrated, Gaia-source-level QSO candidate catalog for selected fields, designed as a high-purity input catalog for fiber-spectroscopic follow-up rather t…

astro-ph.GA2025

Building a Radio AGN Sample from Cosmic Morning -- The Radio High-Redshift Quasar Catalog (RHzQCat): I. Catalog from SDSS Quasars and Radio Surveys at

Yingkang Zhang, Ruqiu Lin, Krisztina Perger +5

Radio-loud high-redshift quasars (RHRQs) provide crucial insights into the evolution of relativistic jets and their connection to the growth of supermassive black holes. Beyond the…

astro-ph.HE2025

A pilot VLBI study of the SQUAB quasar sample featuring multiple Gaia detections

Yingkang Zhang, Tao An, Xiang Ji +5

Our previous work identified a class of SDSS quasars exhibiting multiple Gaia detections, classifying them as candidates for various astrophysical systems such as quasar-star pairs…