Optical design of imaging and spectrograph for 4m telescope in China | |
Hangxin Ji1,2; Yongtian Zhu1,2; Zhongwen Hu1,2; Yi Chen1,2; Lei Wang1,2; Mingming Xu1,2; Songxin Dai1,2; Huatao Zhang1,2 | |
2018-07-06 | |
会议名称 | SPIE Ground-based and Airborne Instrumentation for Astronomy VII(VOL.10702) |
会议录名称 | Ground-based and Airborne Instrumentation for Astronomy VII |
会议日期 | 2018-6-10 |
会议地点 | Austin, Texas, United States |
摘要 |
The design and performance of a three-channel image and long-slit spectrograph for the new 4-m telescope in China are described. The direct imaging covers a 3 arcmin by 3 arcmin field of view and a large wavelength range 370-1,600 nm, it has two optical channels and one near infrared channel with different filters. The spectrograph with a long slit is to provide two observing modes including the following spectral resolutions: R1000 and R5000. For dispersing optical elements it use volume-phased holographic grisms (VPHG) at each of the spectroscopic modes to simplify the camera system. The low resolution mode (R1000) is provided by consecutive observations with the spectral ranges: 360-860 nm, however it adopts only one VPHG for the first light. The spectral range of medium resolution mode (R5000) is 460-750nm, it is constrained with the use of a 4k × 4k CCD detector of 15 μm pixel size. Peak efficient in the spectrograph are achieved to be higher than 50% in different resolution mode. |
关键词 | Imaging And Spectrograph Three-channel Imaging Low And Medium Resolution Spectrograph Vphg |
学科领域 | 天文技术与方法 |
语种 | 英语 |
文献类型 | 会议论文 |
条目标识符 | http://ir.niaot.ac.cn/handle/114a32/1555 |
专题 | 会议论文 |
作者单位 | 1.南京天文光学技术研究所 2.天文光学技术重点实验室 |
推荐引用方式 GB/T 7714 | Hangxin Ji,Yongtian Zhu,Zhongwen Hu,et al. Optical design of imaging and spectrograph for 4m telescope in China[C],2018. |
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文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
Optical design of im(1529KB) | 会议论文 | 开放获取 | CC BY-NC-SA | 浏览 下载 |
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