collaborators

5 papers

astro-ph.CO2026

Prospects for probing dark matter with filamentary 21cm emission

Yizhou Liu, Yingjie Jing, Haoran Shi +1

The cosmic web contains most of the matter in the Universe, and its filamentary structure is closely related to the properties of dark matter. Compared with the cold dark matter (C…

astro-ph.CO2026

Distinguishing the nature of dark matter by mapping cosmic filaments from Lyman-alpha emission

Yizhou Liu, Liang Gao, Shihong Liao +3

The standard CDM cosmological model predicts that cosmic filaments are highly clumpy, whereas warm dark matter -- invoked to address small-scale challenges in CDM -- produces…

astro-ph.CO2025

Detection of HI filament: Pair Stacking vs. Filament Stacking

Yuxi Meng, Jie Wang, Yingjie Jing +2

The faint 21 cm signal emitted by neutral hydrogen in cosmic filaments is expected to be detectable. However, due to its weakness, stacking techniques are required. We assessed two…

astro-ph.GA2025

The impact of cosmic filaments on the abundance of satellite galaxies

Yuxi Meng, Haonan Zheng, Shihong Liao +9

The impact of cosmic web environments on galaxy properties plays a critical role in understanding galaxy formation. Using the state-of-the-art cosmological simulation IllustrisTNG,…

astro-ph.GA2025

Formation of the dark-matter deficient S0 galaxy NGC 4111 under the tidal interactions

Mei Ai, Ming Zhu, Nai-ping Yu +8

We present the high-sensitivity and large-scale atomic hydrogen (HI) observations towards lenticular (S0) galaxy NGC 4111 using the Five-hundred-meter Aperture Spherical Radio Tele…