activity
20222025
most citedA new method of reconstructing Galactic three-dimensional structures using ultralong-wavelength radio observations

6 citations · 12 across the 6 of their papers we have counts for

collaborators

6 papers

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.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

Loop I/NPS morphology predictions in the ultralong-wavelength band

Yanping Cong, Bin Yue, Yidong Xu +3

Loop I/North Polar Spur (NPS) is the giant arc structure above the Galactic plane observed at radio wavelengths ( GHz). There has been long-standing debate about its o…

astro-ph.IM2024★ 3 cited

Forecast measurement of the 21 cm global spectrum from Lunar orbit with the Vari-Zeroth-Order Polynomial (VZOP) method

Tianyang Liu, Jiajun Zhang, Yuan Shi +7

The cosmic 21 cm signal serves as a crucial probe for studying the evolutionary history of the Universe. However, detecting the 21 cm signal poses significant challenges due to its…

astro-ph.GA2024

Galmoss: A package for GPU-accelerated Galaxy Profile Fitting

Mi Chen, Rafael S. de Souza, Quanfeng Xu +5

We introduce galmoss, a python-based, torch-powered tool for two-dimensional fitting of galaxy profiles. By seamlessly enabling GPU parallelization, galmoss meets the high computat…

astro-ph.GA2022★ 6 cited

A new method of reconstructing Galactic three-dimensional structures using ultralong-wavelength radio observations

Yanping Cong, Bin Yue, Yidong Xu +2

The free-free absorption of low frequency radio waves by thermal electrons in the warm ionized medium of our Galaxy becomes very significant at MHz (ultralong-wavelen…