collaborators

9 papers

gr-qc2026

Two-Dimensional Pulsar Distance Inference from Nanohertz Gravitational Waves

Si-Ren Xiao, Ji-Yu Song, Yue Shao +3

Pulsar timing arrays (PTAs) are limited in localizing nanohertz continuous gravitational waves (CGWs) by uncertainties in pulsar distances. We introduce a method to infer pulsar di…

astro-ph.CO2026

Exploring the Cosmic Dawn through the 21 cm Forest and High-redshift Radio Sources with the SKA

Junsong Cang, Benedetta Ciardi, Barun Maity +12

The 21~cm forest, seen as absorption features in the spectra of distant radio sources, is produced by intervening neutral hydrogen and offers a direct probe of the neutral intergal…

astro-ph.CO2026

21 cm forest one-dimensional power spectrum as an indirect probe of dark matter particles and primordial black holes

Meng-Lin Zhao, Yue Shao, Sai Wang +1

Understanding the nature of dark matter (DM) particles remains a pivotal challenge in modern cosmology. Current cosmological research on these phenomena primarily utilizes cosmic m…

astro-ph.CO2025

Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method

Yue Shao, Tian-Yang Sun, Meng-Lin Zhao +1

The 21-cm forest, composed of spectral absorption features from high-redshift background radio sources, provides a unique probe for studying small-scale structures during the epoch…

astro-ph.CO2025

Analyzing the 21cm forest with Wavelet Scattering Transform: Insight into non-Gaussian features of the 21cm forest

Hayato Shimabukuro, Yidong Xu, Yue Shao

The 21cm forest, narrow absorption features in the spectra of high redshift radio sources caused by intervening neutral hydrogen, offers a unique probe of the intergalactic medium…

astro-ph.CO2025

Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens

Ling-Feng Wang, Yue Shao, Si-Ren Xiao +2

Ultra-low-frequency gravitational waves (GWs) generated by individual inspiraling supermassive black hole binaries (SMBHBs) at the centers of galaxies may be detected by pulsar tim…