中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Development of the Multi-channel Photometric Survey Telescope

文献类型:会议论文

作者Yuan XY(袁祥岩); Li ZY(李正阳); Niu DS(牛冬生); Lu QS(陆启帅); Jiang FH(姜方华); Wang YF(王跃飞); Li XY(李晓燕); Liang YJ(梁永军)
出版日期2020-12
会议日期2020-12-13
会议地点California, United States
关键词Optical Telescope, Multi-channel Survey Image Quality Calibration
英文摘要
The Multi-channel Photometric Survey Telescope (Mephisto) is a wide-field ground based telescope with a 1.6m primary mirror and 2° field of view, proposed by Yunnan University. The telescope will be capable of imaging the northern sky in three colors simultaneously and deliver a colored movie of the universe. The R-C system with lens corrector was adopted as the optical system considering of the image quality requirement, light obscuration and camera arrangement, in which three cubic splitters were adopted for the three channel beams in order to get satisfied image quality over the whole field of view. Dichroic coating on the cubic will lead to nonuniform efficiency on the focal plane due to the polarization problem and wide incident angle, which need calibration. The image quality represented in 80% encircled light energy is around 0.6arcsec. In order to keep the optimal image quality in any operational conditions, a 5-DOF mechanism was designed to actively adjust M2 mirror positions according to the wavefront sensors or by direct star psf. Now the telescope are under developing in Nanjing, expected to be installed at Lijiang observatory before the end of 2021.
会议录Proc. SPIE 11445
学科主题天文技术与方法
语种英语
源URL[http://ir.niaot.ac.cn/handle/114a32/1773]  
专题会议论文
作者单位南京天文光学技术研究所
推荐引用方式
GB/T 7714
Yuan XY,Li ZY,Niu DS,et al. Development of the Multi-channel Photometric Survey Telescope[C]. 见:. California, United States. 2020-12-13.

入库方式: OAI收割

来源:南京天文光学技术研究所

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。