Study of photometric phase curve： assuming a cellinoid ellipsoid shape for asteroid （106） Dione
- ISSN号：1674-4527
- 期刊名称：《天文和天体物理学研究：英文版》
- 时间：0
- 分类：P185.7[天文地球—天文学] TP391.41[自动化与计算机技术—计算机应用技术;自动化与计算机技术—计算机科学与技术]
- 作者机构：[1]Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China, [2]University of Chinese Academy of Sciences, Beijing 100049, China, [3]Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, China, [4]Center for Astronomical Mega-Science, Chinese Academy of Sciences, Beijing 100012, China, [5]Sugarloaf Mountain Observatory, South Deerfield, MA 01373, USA
- 相关基金：We thank the referees for their insightful comments and suggestions that lead to significant improvements in this work. We gratefully acknowledge the computing time granted by Yunnan Observatories and provided on the facilities at the Yunnan Observatories Supercomputing Platform. This work is funded by the National Natural Science Foundation of China （Grant Nos. 11073051, 11473066 and 11673063） and by the Open Project of Key Laboratory of Space Object and Debris Observation, Chinese Academy of Sciences （title： Photometric study of space debris in near geostationary orbit）.
关键词：
相位曲线, 小行星, 椭球形, 光度, 二酮, 亮度模式, 观测数据, 函数系统, asteroids, general, photometric phase curve -- asteroids, individual, （106） Dione - techniques： photometric - Markov Chain Monte Carlo method
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