93 citations · 123 across the 5 of their papers we have counts for
10 papers · 1 filter
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…
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…
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…
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…
Automation of the AST3 optical sky survey from Dome~A, Antarctica
Bin Ma, Yi Hu, Zhaohui Shang +6
The 0.5\,m Antarctic Survey Telescopes (AST3) were designed for time-domain optical/infrared astronomy. They are located in Dome~A, Antarctica, where they can take advantage of the…
Multi-star Turbulence Monitor: A new technique to measure optical turbulence profiles
Paul Hickson, Bin Ma, Zhaohui Shang +1
The strength and vertical distribution of atmospheric turbulence is a key factor determining the performance of optical and infrared telescopes, with and without adaptive optics. Y…