Metrology Camera System of Prime Focus Spectrograph for Subaru Telescope
| Autor: | Atsushi Shimono, Hung-Hsu Ling, Hiroshi Karoji, Chi-Hung Yan, Peter H. Mao, Hsin-Yo Chen, Youichi Ohyama, James E. Gunn, Richard C. Y. Chou, Shiang-Yu Wang, Naoyuki Tamura, Jennifer L. Karr, Yen-Sang Hu, Pin-Jie Huang, Naruhisa Takato, Hajime Sugai, Yin-Chang Chang |
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| Přispěvatelé: | Ramsay, Suzanne K., McLean, Ian S., Takami, Hideki |
| Rok vydání: | 2014 |
| Předmět: |
Physics
CMOS sensor business.industry Aperture Astrophysics::Instrumentation and Methods for Astrophysics Cassegrain reflector Physics::Optics FOS: Physical sciences Astrophysics::Cosmology and Extragalactic Astrophysics Metrology Optics Cardinal point Astrophysics::Earth and Planetary Astrophysics Astrophysics - Instrumentation and Methods for Astrophysics business Focus (optics) Subaru Telescope Spectrograph Instrumentation and Methods for Astrophysics (astro-ph.IM) Astrophysics::Galaxy Astrophysics |
| DOI: | 10.48550/arxiv.1408.2876 |
| Popis: | The Prime Focus Spectrograph (PFS) is a new optical/near-infrared multi-fiber spectrograph designed for the prime focus of the 8.2m Subaru telescope. The metrology camera system of PFS serves as the optical encoder of the COBRA fiber motors for the configuring of fibers. The 380mm diameter aperture metrology camera will locate at the Cassegrain focus of Subaru telescope to cover the whole focal plane with one 50M pixel Canon CMOS sensor. The metrology camera is designed to provide the fiber position information within 5{\mu}m error over the 45cm focal plane. The positions of all fibers can be obtained within 1s after the exposure is finished. This enables the overall fiber configuration to be less than 2 minutes. Comment: 10 pages, 12 figures, SPIE Astronomical Telescopes and Instrumentation 2014 |
| Databáze: | OpenAIRE |
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