activity
20242026
collaborators

5 papers

astro-ph.CO2026

Brightest Cluster Galaxy ellipticity as proxy for halo shape: Orientation bias, assembly bias, and potential selection effects in SZ-selected clusters

Radhakrishnan Srinivasan, Tae-hyeon Shin, Anja von der Linden +93

The orientation of triaxial galaxy clusters with respect to the line-of-sight is expected to be one of the prime sources of scatter and potential bias in optical observables (e.g.,…

astro-ph.GA2026

The Fate of the Milky Way--Andromeda System: To Merge or Not?

Hao Wu, Yang Huang, Huawei Zhang +2

It has long been predicted that the Milky Way (MW) will eventually merge with Andromeda (M31), a view reinforced by \textit{HST} measurements indicating a small M31 transverse velo…

astro-ph.GA2025

Revisiting the Proper Motions of M31 and M33 Using Massive Supergiant Stars with Gaia DR3

Hao Wu, Yang Huang, Huawei Zhang +1

The proper motions (PMs) of M31 and M33 are key to understanding the Local Group's dynamical evolution. However, measurement discrepancies between Gaia blue and red samples, regard…

astro-ph.GA2025

Finding Quasars Behind the Galactic Plane: Spectroscopic Identifications of ~1300 New Quasars at |b|<=20 degree from LAMOST DR10

Zhi-Ying Huo, Yuming Fu, Yang Huang +10

Quasars behind the Galactic plane (GPQs) are excellent tracers to probe the chemistry and kinematics of the interstellar/intergalactic medium (ISM/IGM) of the Milky Way along sight…

astro-ph.GA2024

The LAMOST Spectroscopic Survey of Supergiants in M31 and M33

Hao Wu, Yang Huang, Huawei Zhang +3

We present systematic identifications of supergiants of M31/M33 based on massive LAMOST spectroscopic survey. Radial velocities of nearly 5000 photometrically selected M31/M33 supe…