activity
20072024
most citedThe Bulge Radial Velocity Assay (BRAVA): II. Complete Sample and Data Release

244 citations · 1.1k across the 48 of their papers we have counts for

collaborators

49 papers

astro-ph.IM2024★ 3 cited

The Electrical Design of a Membrane Antenna for Lunar-based Low-frequency Radio Telescope

Suonanben, Fengquan Wu, Kai He +15

Detecting primordial fluctuations from the cosmic dark ages requires extremely large low-frequency radio telescope arrays deployed on the far side of the Moon. The antenna of such…

astro-ph.IM2024

The FRB-searching pipeline of the Tianlai Cylinder Pathfinder Array

Zijie Yu, Furen Deng, Shijie Sun +14

This paper presents the design, calibration, and survey strategy of the Fast Radio Burst (FRB) digital backend and its real-time data processing pipeline employed in the Tianlai Cy…

astro-ph.IM2024★ 19 cited

Large-scale Array for Radio Astronomy on the Farside

Xuelei Chen, Feng Gao, Fengquan Wu +20

At the Royal Society meeting in 2023, we have mainly presented our lunar orbit array concept called DSL, and also briefly introduced a concept of a lunar surface array, LARAF. As t…

astro-ph.IM2023

Application of Regularization Methods in the Sky Map Reconstruction of the Tianlai Cylinder Pathfinder Array

Kaifeng Yu, Shifan Zuo, Fengquan Wu +2

The Tianlai cylinder pathfinder is a radio interferometer array to test 21 cm intensity mapping techniques in the post-reionization era. It works in passive drift scan mode to surv…

astro-ph.IM2023

A simulation of calibration and map-making errors of the Tianlai cylinder pathfinder array

Kaifeng Yu, Fengquan Wu, Shifan Zuo +4

The Tianlai cylinder array is a pathfinder for developing and testing 21cm intensity mapping techniques. In this paper, we use numerical simulation to assess how its measurement is…

astro-ph.GA2023★ 5 cited

Mapping the Milky Way's stellar halo with 2D data

Anda Chen, Zhigang Li, Yougang Wang +3

We propose a new method for measuring the spatial density distribution of the stellar halo of the Milky Way. Our method is based on a pairwise statistic of the distribution of star…