A New Fiber Detection Method for LAMOST Based on the Front-illuminated Method. (1st June 2022)
- Record Type:
- Journal Article
- Title:
- A New Fiber Detection Method for LAMOST Based on the Front-illuminated Method. (1st June 2022)
- Main Title:
- A New Fiber Detection Method for LAMOST Based on the Front-illuminated Method
- Authors:
- Zhou, Ming
Zhang, Yong
Lv, Guanru
Li, Jian
Zhou, Zengxiang
Liu, Zhigang
Wang, Jianping
Bai, Zhongrui
Tian, Yuan
Wang, Mengxin
Wang, Shuqing
Hu, Hongzhuan
Zhai, Chao
Chu, Jiaru
Han, Zhijie
Liu, Mingxu
Dong, Yiqiao
Yuan, Hailong
Zhao, Yongheng
Chu, Yaoquan
Zhang, Haotong - Abstract:
- Abstract: The double revolving fiber positioning technology is one of the key technologies for the success of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST). The accuracy of fiber positioning will directly affect the observation efficiency of LAMOST. To achieve higher fiber positioning accuracy, the original open-loop controlled fiber positioning system urgently needs to be upgraded into a closed-loop control system. The fiber detection is the most important part of the closed-loop controlled fiber positioning system. The back-illuminated detection method is usually used to detect the fiber position by directly detecting the light spot generated at the fiber end in the multi-fiber spectral surveys. In this paper, we introduce a new method to measure the fiber position based on the image of the front-illuminated LAMOST focal plane. The front-illuminated image does not require lighting devices inside the spectrograph, and it could reduce the instability and light pollution in the spectrograph end. Our method measures the fiber position by fitting the profile of the fiber pinhole with a 2D Gaussian function. A series of tests show that the relative position measurement precision of the front-illuminated method is about 0.″12, and the method could have the same accuracy as the back-illuminated method once the system bias is calibrated by a simple radial correction function. The required fiber positioning accuracy of LAMOST is 0.″4, and the new methodAbstract: The double revolving fiber positioning technology is one of the key technologies for the success of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST). The accuracy of fiber positioning will directly affect the observation efficiency of LAMOST. To achieve higher fiber positioning accuracy, the original open-loop controlled fiber positioning system urgently needs to be upgraded into a closed-loop control system. The fiber detection is the most important part of the closed-loop controlled fiber positioning system. The back-illuminated detection method is usually used to detect the fiber position by directly detecting the light spot generated at the fiber end in the multi-fiber spectral surveys. In this paper, we introduce a new method to measure the fiber position based on the image of the front-illuminated LAMOST focal plane. The front-illuminated image does not require lighting devices inside the spectrograph, and it could reduce the instability and light pollution in the spectrograph end. Our method measures the fiber position by fitting the profile of the fiber pinhole with a 2D Gaussian function. A series of tests show that the relative position measurement precision of the front-illuminated method is about 0.″12, and the method could have the same accuracy as the back-illuminated method once the system bias is calibrated by a simple radial correction function. The required fiber positioning accuracy of LAMOST is 0.″4, and the new method satisfies the requirement of LAMOST fiber detection accuracy and could be used in the closed-loop fiber control system. … (more)
- Is Part Of:
- Research in astronomy and astrophysics. Volume 22:Number 6(2022)
- Journal:
- Research in astronomy and astrophysics
- Issue:
- Volume 22:Number 6(2022)
- Issue Display:
- Volume 22, Issue 6 (2022)
- Year:
- 2022
- Volume:
- 22
- Issue:
- 6
- Issue Sort Value:
- 2022-0022-0006-0000
- Page Start:
- Page End:
- Publication Date:
- 2022-06-01
- Subjects:
- techniques: image processing -- methods: data analysis -- instrumentation: detectors
Astronomy -- Periodicals
Astrophysics -- Periodicals
520.5 - Journal URLs:
- http://iopscience.iop.org/1674-4527 ↗
- DOI:
- 10.1088/1674-4527/ac6734 ↗
- Languages:
- English
- ISSNs:
- 1674-4527
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library STI - ELD Digital store
- Ingest File:
- 23237.xml