USTC Briefing Interests and overlaps

来源 :中国-国际三十米望远镜天文台合作会议(TMT WFOS China Partnership meeting) | 被引量 : 0次 | 上传用户:lovegoodone
下载到本地 , 更方便阅读
声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架
论文部分内容阅读
USTC TMT Team Members Zhai,Chao:Mechanial Engineering Wang,Jianping:Mechanical Engineering Hu,Hongzhuan:Mechanical Engineering Qiu,Keqiang:Grating Fabrication Wang,Jian:Electronic and Software Engineering Zhu,Qingfeng:Astronomical Instrumentation
其他文献
碳酸盐岩、致密砂岩等渗透性较低、流体性质识别难的复杂气藏,常规测井很难准确地对其进行评价.阵列声波测井包含着丰富的地层信息,在渗透性评价和流体识别方面表现出独特的
OUTLINE ·Introduction of Sub-Millimeter Array(SMA)·New SMA Receiver – wSMA·Current status of wSMA·Conclusions OUTLINE
会议
本文首先对LAMOST巡天数据进行了简单回顾,并对数据产品中恒星参数的精度进行分析,最后举例说明了海量天体光谱数据挖掘的结果。
将天文光梳顺利安装在2.16米望远镜现场;研究了散斑噪声对天文光梳定标精度的影响,采用OCT光纤配合动态扰模对散斑噪声进行了有效抑制;在216HRS光谱仪上,天文光梳的短期定标精度
TAOS Ⅱ the Transneptunian Automated Occultation Survey,will measure the size distribution of small objects(~1 km diameter) in the Kuiper Belt and beyond.
会议
OUTLINE I.INTRODUCTION CCD CONTROLLER AND TWO ASIC devices The controller configuration II.SPA DESIGN AND PERFORMANCES OF SPA The goals of the SPA Noise:
会议
SHAO:introduction Departments:Center for Astro-geodynamics Division of Astrophysics Division of Radio Astronomy Science and Technology Division of Optical Astro
会议
Contents 1 WFOS-MOBIE SYS Mini-study 2 SJTU-team projects relevant to WFOS 3 Overlaps with WFOS challenges WFOS-MOBIE SYS Mini-Study SYS Mini-study Matt Radovan
会议
Outlook What is PTST?Observatorio astronómico de la Sagra The telescope Fast imaging Observations Summary
会议
首次在国际上建立天区面积最大、星等最深、数目最多的高信噪比中分辨率恒星光谱库,视向速度和恒星参数的测量精度分别提高5倍和1倍,并可测得10多种元素的丰度,有望在银河系和恒