activity
20142026
most citedOptical Observations of LIGO Source GW 170817 by the Antarctic Survey Telescopes at Dome A, Antarctica

96 citations · 410 across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.IM2026

Atmospheric turbulence profiling with the Multistar Turbulence Monitor

Weisen Huang, Bin Ma, Tengfei Song +5

Accurate characterization of atmospheric optical turbulence is essential for evaluating astronomical sites and optimizing adaptive optics systems. The Multistar Turbulence Monitor…

astro-ph.IM2023

Machine learning-based seeing estimation and prediction using multi-layer meteorological data at Dome A, Antarctica

Xu Hou, Yi Hu, Fujia Du +6

Atmospheric seeing is one of the most important parameters for evaluating and monitoring an astronomical site. Moreover, being able to predict the seeing in advance can guide obser…

astro-ph.SR2023★ 5 cited

Data Release of the AST3-2 Automatic Survey from Dome A, Antarctica

Xu Yang, Yi Hu, Zhaohui Shang +18

AST3-2 is the second of the three Antarctic Survey Telescopes, aimed at wide-field time-domain optical astronomy. It is located at Dome A, Antarctica, which is by many measures the…

astro-ph.IM2020★ 17 cited

Cloud Cover and Aurora Contamination at Dome A in 2017 from KLCAM

Xu Yang, Zhaohui Shang, Keliang Hu +6

Dome A in Antarctica has many characteristics that make it an excellent site for astronomical observations, from the optical to the terahertz. Quantitative site testing is still ne…

astro-ph.IM2020

NBFTP: A Dedicated Data Transfer System for Remote Astronomical Observation at Dome A

Siyuan Huang, Ce Yu, Chao Sun +5

Dome A, Antarctica has been thought to be one of the best astronomical sites on the earth since decades ago. From it was first visited by astronomers in 2008, dozens of facilities…

astro-ph.IM2020★ 93 cited

Night-time measurements of astronomical seeing at Dome A in Antarctica

Bin Ma, Zhaohui Shang, Yi Hu +6

Seeing, the angular size of stellar images blurred by atmospheric turbulence, is a critical parameter used to assess the quality of astronomical sites. Median values at the best mi…