collaborators

15 papers

astro-ph.IM2026

21 cm Power Spectrum Analysis of North Celestial Pole Observations with the Tianlai Dish Pathfinder Array

Guangzhi He, Shifan Zuo, Jixia Li +11

The Tianlai Dish Pathfinder Array (TDPA) is a radio interferometer designed to test techniques for 21 cm intensity mapping in the post-reionization universe as a means of measuring…

astro-ph.CO2026

Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies

Ya-Nan Du, Ji-Yu Song, Yichao Li +4

Gravitational-wave (GW) events are generally believed to originate in galaxies and can thus serve, like galaxies, as tracers of the universe's large-scale structure. In GW observat…

astro-ph.HE2026

Unveiling the spectral morphological division of fast radio bursts with CHIME/FRB Catalog 2

Wan-Peng Sun, Yin-Long Cao, Yong-Kun Zhang +7

Fast radio bursts (FRBs) are commonly classified into repeating and apparently nonrepeating sources, yet whether this distinction reflects intrinsically different physical populati…

astro-ph.HE2026

A Practical Framework for Estimating the Repetition Likelihood of Fast Radio Bursts from Spectral Morphology

Wan-Peng Sun, Yong-Kun Zhang, Ji-Guo Zhang +6

The repeating behavior of fast radio bursts (FRBs) is regarded as a key clue to understanding their physical origin, yet reliably distinguishing repeaters from apparent non-repeate…

astro-ph.CO2025

CMB delensing with deep learning

Shulei Ni, Yichao Li, Xin Zhang

The cosmic microwave background (CMB) stands as a pivotal source for studying weak gravitational lensing. While the lensed CMB aids in constraining cosmological parameters, it simu…

astro-ph.CO2025

Prospects for cosmological research using hundred-meter-class radio telescopes: 21-cm intensity mapping survey strategies with QTT, JRT, and HRT

Jun-Da Pan, Yichao Li, Guo-Hong Du +2

Understanding dark energy requires precision measurements of the expansion history of the universe and the growth of large-scale structure. The 21 cm intensity mapping (21 cm IM) t…