activity
20162020
most citedGPU-Based High-Performance Imaging for Mingantu Spectral RadioHeliograph

12 citations · 28 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2020★ 6 cited

Robust Automated Photometry Pipeline for Blurred Images

Weirong Huang, Zhou Xie, Wenjie Zhong +4

The primary task of the 1.26-m telescope jointly operated by the National Astronomical Observatory and Guangzhou University is photometric observations of the g, r, and i bands. A…

astro-ph.IM2017★ 12 cited

GPU-Based High-Performance Imaging for Mingantu Spectral RadioHeliograph

Ying Mei, Feng Wang, Wei Wang +6

As a dedicated solar radio interferometer, the MingantU SpEctral RadioHeliograph (MUSER) generates massive observational data in the frequency range of 400 MHz -- 15 GHz. High-perf…

astro-ph.IM2017★ 2 cited

High Performance Negative Database for Massive Data Management System of The Mingantu Spectral Radioheliograph

Congming Shi, Feng Wang, Hui Deng +3

As a dedicated synthetic aperture radio interferometer, the MingantU SpEctral Radioheliograph (MUSER), initially known as the Chinese Spectral RadioHeliograph (CSRH), has entered t…

astro-ph.IM2017★ 8 cited

OpenCluster: A Flexible Distributed Computing Framework for Astronomical Data Processing

Shoulin Wei, Feng Wang, Hui Deng +7

The volume of data generated by modern astronomical telescopes is extremely large and rapidly growing. However, current high-performance data processing architectures/frameworks ar…

astro-ph.IM2016

NVST data archiving system based on fastbit nosql database

Yingbo Liu, Feng Wang, Kaifan Ji +3

The New Vacuum Solar Telescope (NVST) is a 1-meter vacuum solar telescope that aims to observe the fine structures of active regions on the Sun. The main tasks of the NVST are high…

astro-ph.IM2016

Low-cost high performance distributed data storage for multi-channel observations

Ying-bo Liu, Feng Wang, Hui Deng +5

The New Vacuum Solar Telescope (NVST) is a 1-m solar telescope that aims to observe the fine structures in both the photosphere and the chromosphere of the Sun. The observational d…