collaborators

13 papers

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…

astro-ph.CO2025

Exploring HI Galaxy Redshift Survey Strategies for the FAST Core Array Interferometry

Zhenglong Li, Diyang Liu, Chengliang Xu +2

We explore the feasibility of HI galaxy redshift surveys with the Five-hundred-meter Aperture Spherical Telescope (FAST) and its proposed Core Array interferometry. Using semi-anal…

astro-ph.CO2025

Deep learning-driven likelihood-free parameter inference for 21-cm forest observations

Tian-Yang Sun, Yue Shao, Yichao Li +3

The hyperfine structure absorption lines of neutral hydrogen in spectra of high-redshift radio sources, known collectively as the 21-cm forest, have been demonstrated as a sensitiv…

astro-ph.IM2025

FAST Drift Scan Survey for HI Intensity Mapping. II. Stacking-based Beam Construction of the 19-feed Array at GHz

Xinyang Zhao, Yichao Li, Wenxiu Yang +7

Neutral hydrogen (HI) intensity mapping (IM) presents great promise for future cosmological large-scale structure surveys. However, a major challenge for HIIM cosmological studies…

astro-ph.CO2025

FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking

Diyang Liu, Yichao Li, Denis Tramonte +5

Filaments stand as pivotal structures within the cosmic web. However, direct detection of the cold gas content of the filaments remains challenging due to its inherent low brightne…