中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The current status of the imaging and spectrogragh (IMSP) for 4m telescope

文献类型:会议论文

作者Ji HX(季杭馨); Chen Y(陈忆); Wang L(王磊); Dai SX(戴松新); Zhang HT(章华涛); Tang Z(汤振); Li J(李军); 新其其格; Zhu YT(朱永田)
出版日期2020-12
会议日期2020-12-13
会议地点California, United States
关键词Imaging And Spectrograph k Mirror Low And Medium Resolution Spectrograph Vphg De-rotator
英文摘要
IMSP is the versatile rst-light instrument under construction for the 4m telescope in China. The special feature of IMSP is the multimode operation modes and high-e ciency. Direct imaging mode is designed to work in a synchronous multi-color bands covering from 360 to 1700 nm using two dichroic mirrors with a 3'x3' eld of view (FOV). Long-slit spectrograph mode supports two spectral resolutions operation modes (R=1000 & 5000) via di erent combination of Volume Phase Holographic Prisms to cover the whole spectrum in visible. High resolution spectrograph mode (R=30000-60000) with wavelength range from 380 to 800 nm is reserved using ber link system connected from Nasmyth foci to the enviroment controled room. The IMSP is planned to strart commssion at the end of 2021. In this paper, the lastest status of IMSP development will be given, including the nal optical design and the integration of each sub-system.
会议录Proc. of SPIE Vol. 11447
学科主题天文技术与方法
语种英语
源URL[http://ir.niaot.ac.cn/handle/114a32/1781]  
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
Ji HX,Chen Y,Wang L,et al. The current status of the imaging and spectrogragh (IMSP) for 4m 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。