Prime Focus Spectrograph (PFS) for the Subaru telescope: A next-generation facility instrument of the Subaru telescope has started coming

Naoyuki Tamura,Naruhisa Takato,Yuki Moritani,Kiyoto Yabe,Yuki Ishizuka, Yukiko Kamata, Ali Allaoui,Stéphane Arnouts, Robert H. Barkhouser, Philippe Balard, Rudy Barette,Mohamed Belhadi, Jill Burnham,Neven Caplar, Michael A. Carr, Pierre Yves Chabaud, Yin Chang Chang, Hsin Yo Chen, Chueh Yi Chou,You-Hua Chu,Judith G. Cohen, Ricardo Costa, Thibaut Crahchet, Rodrigo P. de Almeida,Antonio Cesar de Oliveira,Ligia Souza de Oliveira,Kjetil Dohlen,Leandro Henrique dos Santos,Richard S. Ellis,Maximilian Fabricius,Décio Ferreira,Hisanori Furusawa, Javier Garcia-Carpio, M. Golebiowski,Aidan Gray,James E. Gunn, Randolph Hammond, Albert Harding,Murdock Hart,Timothy M. Heckman, Stephen C. Hope, Shu Fu Hsu, Yen Shan Hu, Ping Jie Huang, M. Jaquet,Eric Jeschke,Yipeng Jing,Erin Kado-Fong,Jennifer L. Karr,Satoshi Kawanomoto,Masahiko Kimura,Michitaro Koike,Eiichiro Komatsu, S. Koshida,Vincent Le Brun,Olivier Le Fèvre, Arnaud Le Fur,David Le Mignant, Hung Hsu Ling,Craig P. Loomis,Robert H. Lupton, F. Madec,Danilo Marchesini, Edouard Marguerite,Lucas Souza Marrara,Dmitry Medvedev,Sogo Mineo,Hitoshi Murayama,Graham J. Murray,Youichi Ohyama,Hirofumi Okita,Yuki Okura,Masato Onodera, Joe D. Orndorff,Sandrine Pascal,Joshua Peebles, Lucio Ramos,Daniel J. Reiley,Martin Reinecke, Mitsuko Roberts, Josimar A. Rosa,Julien Rousselle, Mira Sarkis,Alain Schmitt,Michael Seiffert, Kiaina Schubert,Hassan Siddiqui, Stephen A. Smee,Laerte Sodré,Michael A. Strauss,Christian Surace,Manuchehr Taghizadeh Popp,Philip J. Tait,Masahiro Takada,Satoshi Takita

Ground-Based and Airborne Instrumentation for Astronomy VIII 2020(2021)

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摘要
PFS (Prime Focus Spectrograph), a next generation facility instrument on the Subaru telescope, is a very wide- field, massively multiplexed, and optical and near-infrared spectrograph. Exploiting the Subaru prime focus, 2394 reconfigurable fibers will be distributed in the 1.3 degree-diameter field of view. The spectrograph system has been designed with 3 arms of blue, red, and near-infrared cameras to simultaneously deliver spectra from 380nm to 1260nm in one exposure. The instrumentation has been conducted by the international collaboration managed by the project office hosted by Kavli IPMU. The team is actively integrating and testing the hardware and software of the subsystems some of which such as Metrology Camera System, the first Spectrograph Module, and the first on-telescope fiber cable have been delivered to the Subaru telescope observatory at the summit of Maunakea since 2018. The development is progressing in order to start on-sky engineering observation in 2021, and science operation in 2023. In parallel, the collaboration is trying to timely develop a plan of large-sky survey observation to be proposed and conducted in the framework of Subaru Strategic Program (SSP). This article gives an overview of the recent progress, current status and future perspectives of the instrumentation and scientific operation.
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