Site-testing at Muztagh-ata site II: Seeing statistics

慕士塔格站址选址测试 V：近五年夜间云量

Site-testing at the Muztagh-ata Site.V. Nighttime Cloud Amount during the Last Five Years

该研究基于2017-2021年慕士塔格站址的全天相机数据，统计夜间云量与观测时长，得出年可观测时间占比65%等结论，并对比CLARA数据集分析差异原因，为该台站的天文观测规划提供支撑。

Site-testing at Muztagh-ata site I: Ground Meteorology and Sky Brightness

Site-testing is crucial for achieving the goal of scientific research and analysis of meteorological and optical observing conditions is one of the basic tasks of it. As one of three potential sites to host 12-meter Large Optical/infrared Telescope (LOT), Muztagh-ata site which is located on the Pamirs Plateau in west China's Xinjiang began its site-testing task in the spring of 2017. In this paper, we firstly start with an introduction to the site and then present a statistical analysis of the ground-level meteorological properties such as air temperature, barometric pressure, relative humidi…

慕士塔格观测站观测时间碎片化分析

An analysis of the fragmentation of observing time at the Muztagh-ata site

本文针对慕士塔格站观测时间的碎片化问题，提出 Gamma 函数以综合量化观测时间的比例与连续性，并基于实地数据验证表明该站每年有约 122 个绝对晴朗夜和 205 个极好夜。

帕米尔高原慕士塔格站北1点与北2点的视宁度及气象分析

Seeing and Meteorological Analysis at the North-1 and North-2 Points of Muztagh-Ata Site on the Pamir Plateau

本研究对比分析帕米尔高原慕士塔格站北1、北2点2018-2024年的视宁度与气象数据，证实两地均具备优质大气条件，为中国西部大型光学/红外望远镜选址提供支撑。

ASCNet：穆扎塔格-阿塔天文台全天空相机图像分类研究

ASCNet: Research on all-sky camera images classification at the Muztagh-ata site

ASCNet通过整合ResNet34与ASC模块，利用深度可分离扩张卷积和轻量级注意力机制，实现对全天空相机图像的高精度分类，达到92.7%的一致性率。

Forecast of observing time delay of the strongly lensed quasars with Muztagh-Ata 1.93m telescope

As a completely independent method, the measurement of time delay of strongly lensed quasars (TDSL) are crucial to resolve the Hubble tension. Extensive monitoring is required but so far limited to a small sample of strongly lensed quasars. Together with several partner institutes, Beijing Normal University is constructing a 1.93m reflector telescope at the Muztagh-Ata site in west China, which has the world class observing conditions. The telescope will be equipped with both a three-channel imager/photometer which covers $3500-11000$ Angstrom wavelength band, and a low-medium resolution ($λ/δ…