activity
20222026
most citedLunar Orbit Measurement of Cosmic Dawn 21 cm Global Spectrum

31 citations · 130 across the 48 of their papers we have counts for

collaborators

50 papers

astro-ph.CO2026

Cross-correlating Squared kSZ and HI Intensity Fields: A Map-level ACT--MeerKAT Forecast

Yu-Er Jiang, Yun Liu, Yan Gong +5

The kinetic Sunyaev--Zel'dovich (kSZ) effect probes the line-of-sight momentum of free electrons, but its blackbody spectrum and velocity-dependent sign make it difficult to isolat…

astro-ph.IM2026

Synthesis imaging with a lunar orbit array: III. Augmented lagrangian Multiplier Imaging using Gradient descent Optimization (AMIGO)

Meng Zhou, Furen Deng, Yidong Xu +1

Ground-based radio observations below 30 MHz are severely limited by ionospheric interference and radio frequency interference (RFI) from Earth. A lunar-orbiting radio interferomet…

astro-ph.GA2026

A Statistical Study of HI Gas in AGN-Hosting and Satellite Galaxies from ALFALFA and FASHI

Shuanghao Shu, Wenkai Hu, Junqiang Ge +6

We investigate the relative importance of Active Galactic Nucleus (AGN) feedback and environmental processes using a large sample of HI galaxies from the ALFALFA and FASHI surveys.…

astro-ph.CO2026

Wedge-avoidance Fisher Forecasts for Primordial Features from Dark-Ages 21-cm Power Spectrum and Bispectrum

Chen Zhang, Furen Deng, Yidong Xu +3

The Dark Ages offer a uniquely clean window on primordial physics, making the redshifted 21-cm signal a promising probe of inflation models. Forecasts for interferometric 21-cm mea…

astro-ph.CO2026

A Designer's Guide to Lunar Far-Side Interferometer Array: Power Spectrum Measurement and Cosmological Constraints from the Dark Ages

Yuewei Wen, Bin Yue, Yidong Xu +4

The 21-cm emission line from neutral hydrogen during the cosmic Dark Ages can be a powerful probe of cosmological models and early universe physics. This work provides a quantitati…

astro-ph.GA2026

Cross-Comparison of Galaxies Detected in the CSST Spectroscopic Survey and the SKA HI Survey

Yingfeng Liu, Furen Deng, Wenxiang Pei +8

We present a forward-modeling framework to forecast the galaxies detected in the Chinese Space Station Survey Telescope (CSST) spectroscopic survey and the Square Kilometre Array (…

astro-ph.IM2026

Measuring Tianlai's primary beam using sky model

Yunbo Geng, Furen Deng, Jixia Li +6

We present the beam pattern measurement of the Tianlai Cylinder Pathfinder Array. As it is a pure drift-scan instrument, we exploit the North-South motion of the Sun to demonstrate…

astro-ph.CO2026

Constraining Lyman-Werner Feedback from Velocity Acoustic Oscillations in the Cosmic Dawn 21 cm Signal

Xi Du, Bin Yue, Furen Deng +4

During Cosmic Dawn, Pop III stars could be formed in minihalos through molecular hydrogen (H) cooling. The minimum halo mass required for H cooling is highly sensitive to L…

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

Impact of Stochastic Pop~III X-ray Binaries on the Cosmological 21-cm Signal

Saswata Dasgupta, Boyuan Liu, Anastasia Fialkov +3

High-mass X-ray binaries are one of the primary drivers of the 21-cm signal from Cosmic Dawn and Reionization, playing a leading role in the thermal history of the intergalactic me…

astro-ph.IM2026

Synthesis imaging with a lunar orbit array: II. Impacts of instrument-induced phase errors

Meng Zhou, Furen Deng, Yidong Xu +2

A lunar orbit interferometer array suffers from a number of systematics. Beyond systematics induced by the imaging algorithm itself and thermal noise considered in Paper I, phase e…

astro-ph.GA2026

FATHOMER survey: III. Preliminary HI galaxy identification results

Shuanghao Shu, Yichao Li, Wenxiu Yang +6

We present the HI galaxy observation results of the FATHOMER (FAst neuTral HydrOgen intensity Mapping ExpeRiment), a pilot drift scan survey by the Five-hundred-meter Aperture Sphe…

cs.LG2025

AI Agent for Source Finding by SoFiA-2 for SKA-SDC2

Xingchen Zhou, Nan Li, Peng Jia +7

Source extraction is crucial in analyzing data from next-generation, large-scale sky surveys in radio bands, such as the Square Kilometre Array (SKA). Several source extraction pro…

astro-ph.HE2025

Jet reorientation revealed by intermittent jet activity in radio galaxy 0954+556

Ai-Ling Zeng, Wei Zhao, Jun Yang +9

Intermittent jet activity of AGNs is a common phenomenon, whereas significant jet reorientation during episodic jet activity in relatively young radio galaxies are rarely reported.…

astro-ph.IM2025★ 2 cited

Synthesis imaging with a lunar orbit array: I. global sky map and its systematics

Furen Deng, Yidong Xu, Fengquan Wu +3

Ground-based radio astronomical observation at frequencies below 30 MHz is hampered by the Ionosphere and radio frequency interference (RFI). The Discovering Sky at the Longest wav…

astro-ph.CO2025

The first AKRA mass map reconstruction from HSC Y1 data

Yuan Shi, Pengjie Zhang, Zhao Chen +4

Weak lensing mass-mapping from shear catalogs faces systematic challenges from survey masks and spatially varying noise. To overcome these issues and reconstruct unbiased convergen…

astro-ph.CO2025

Exploring Cosmological Constraints of the Void-Lensing Cross-Correlation in the CSST Photometric Survey

Qi Xiong, Yan Gong, Junhui Yan +8

We investigate the cosmological constraints from the void-lensing cross-correlation assuming the CDM model for the Chinese Space Station Survey Telescope (CSST) photometric surv…

astro-ph.IM2025

Beamforming in Interferometer Arrays with Cross-couplings

Yingfeng Liu, Shijie Sun, Kaifeng Yu +6

For an interferometric array, an image of the sky can be synthesized from interferometric visibilities, which are the cross-correlations of the received electric voltages of pairs…

astro-ph.CO2025

Exploring Joint Observation of the CSST Shear and clustering of astrophysical gravitational wave source measurements

Pengfei Su, Yan Gong, Qi Xiong +4

We present a comprehensive forecast for cosmological constraints using the joint observation of the cosmic shear signal from the Chinese Space Station Survey Telescope (CSST) and t…

astro-ph.CO2025

Cosmological Prediction from the joint observation of MeerKAT and CSST at = 0.4 1.2

Yu-Er Jiang, Yan Gong, Qi Xiong +10

Cross-correlating neutral hydrogen (HI) 21cm intensity mapping with galaxy surveys provides an effective probe of astrophysical and cosmological information. This work presents a c…

astro-ph.IM2025★ 3 cited

GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations

Xingchen Zhou, Hang Yang, Nan Li +11

We introduce GalaxyGenius, a Python package designed to produce synthetic galaxy images tailored to different telescopes based on hydrodynamical simulations. Its implementation wil…

astro-ph.GA2025★ 1 cited

A Multi-Mechanism Hybrid Model of Peaked-Spectrum Radio Sources

Guang-Chen Sun, Yichao Li, Furen Deng +6

The peaked-spectrum (PS) sources exhibit turnover characteristics in their broad radio spectra. However, the mechanism underlying this phenomenon remains elusive. The two most comm…

astro-ph.GA2025

Reconstructing the Anisotropic Ultra-long Wavelength Spectra using a Single Antenna on Lunar-orbit

Qige Ao, Furen Deng, Yidong Xu +3

The ultra-long wavelength sky ( MHz) is still largely unexplored, as the electromagnetic wave is heavily absorbed and distorted by the ionosphere on Earth. The far-si…

astro-ph.CO2025

FAST drift scan survey for HI intensity mapping: simulation on Bayesian-stacking-based HI mass function estimation

Jiaxin Wang, Yichao Li, Hengxing Pan +7

This study investigates the estimation of the neutral hydrogen (HI) mass function (HIMF) using a Bayesian stacking approach with simulated data for the Five-hundred-meter Aperture…