Prime Focus Spectrograph (PFS) for the Subaru Telescope: its start of the last development phase
Prime Focus Spectrograph (PFS) for the Subaru Telescope: its start of the last development phase
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斯巴鲁望远镜的主焦摄谱仪（PFS）：最后一个开发阶段的开始
DOI：
10.1117/12.2628152
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发表时间：
2022
期刊：
影响因子：
--
通讯作者：
Barette, Rudy
中科院分区：
文献类型：
--
作者：
Tamura, Naoyuki;Moritani, Yuki;Yabe, Kiyoto;Ishizuka, Yuki;Kamata, Yukiko;Allaoui, Ali;Arai, Akira;Arnouts, Stéphane;Barkhouser, Robert H.;Barette, Rudy
PFS（Prime Focus Spectrograph）是斯巴鲁望远镜上的下一代设施仪器，目前正在望远镜上进行测试。该仪器在斯巴鲁的主焦点上配备了非常宽（直径1.3度）的视场，2394根可重构光纤的高复用性，以及一次曝光同时覆盖380 nm至1260 nm的宽波段光谱仪。目前，工程观察正在进行中，主要焦点仪器（PFI），计量相机系统（MCS），第一个光谱仪模块（SM 1）与可见光相机和第一个光纤电缆提供PFI和SM 1之间的光学链接。在其余硬件中，第二条光纤电缆已于2022年4月安装在望远镜和圆顶建筑中，另外两条也于2022年6月交付。包括近红外相机在内的下一代SM的集成和测试正在进行中，以便及时交付。软件开发的进展也值得注意。与分系统一起交付的仪器控制软件正在与其系统一级的层、望远镜系统、观测规划软件和相关数据库很好地结合起来。数据简化管道也在迅速进展，特别是自2021年初开始使用斯巴鲁夜空光谱仪（SuNSS）拍摄天空光谱以来，以及最近在工程观测期间使用PFI以来。在这些仪器活动的同时，PFS科学团队正在及时制定一项大天空调查观测计划，该计划将作为斯巴鲁战略计划（SSP）从2024年开始提出并实施。在这篇文章中，我们报告这些最近的进展，正在进行的发展和未来的前景PFS仪器。
PFS (Prime Focus Spectrograph), a next generation facility instrument on the Subaru telescope, is now being tested on the telescope. The instrument is equipped with very wide (1.3 degrees in diameter) field of view on the Subaru’s prime focus, high multiplexity by 2394 reconfigurable fibers, and wide waveband spectrograph that covers from 380nm to 1260nm simultaneously in one exposure. Currently engineering observations are ongoing with Prime Focus Instrument (PFI), Metrology Camera System (MCS), the first spectrpgraph module (SM1) with visible cameras and the first fiber cable providing optical link between PFI and SM1. Among the rest of the hardware, the second fiber cable has been already installed on the telescope and in the dome building since April 2022, and the two others were also delivered in June 2022. The integration and test of next SMs including near-infrared cameras are ongoing for timely deliveries. The progress in the software development is also worth noting. The instrument control software delivered with the subsystems is being well integrated with its system-level layer, the telescope system, observation planning software and associated databases. The data reduction pipelines are also rapidly progressing especially since sky spectra started being taken in early 2021 using Subaru Nigh Sky Spectrograph (SuNSS), and more recently using PFI during the engineering observations. In parallel to these instrumentation activities, the PFS science team in the collaboration is timely formulating a plan of large-sky survey observation to be proposed and conducted as a Subaru Strategic Program (SSP) from 2024. In this article, we report these recent progresses, ongoing developments and future perspectives of the PFS instrumentation.
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影响因子：
2.3
作者：
M. Takada;R. Ellis;M. Chiba;J. Greene;H. Aihara;N. Arimoto;K. Bundy;J. Cohen;O. Dor'e
通讯作者：
M. Takada;R. Ellis;M. Chiba;J. Greene;H. Aihara;N. Arimoto;K. Bundy;J. Cohen;O. Dor'e
ULTIMATE-Subaru：GLAO 初步设计概述
DOI：
10.1117/12.2629749
发表时间：
2022
期刊：
Proceedings of the SPIE
影响因子：
--
作者：
Minowa Yosuke;Ono Yoshito;Tanaka Yoko;Yoshida Hiroshige;Terao Koki;Koyama Yusei;Ali Sadman;Tanaka Ichi;Hattori Takashi;Okita Hirofumi;他20名
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他20名
斯巴鲁望远镜第二代观测控制系统的轻量级容错中间件
DOI：
10.1117/12.788052
发表时间：
2008
期刊：
Ground-based and Airborne Instrumentation for Astronomy VIII
影响因子：
--
作者：
E. Jeschke;B. Bon;Takeshi Inagaki;Sam Streeper
通讯作者：
Sam Streeper
主焦光谱仪 (PFS)：计量相机系统
DOI：
10.1117/12.2561191
发表时间：
2020
期刊：
Ground-based and Airborne Instrumentation for Astronomy VIII
影响因子：
--
作者：
Shiang‐Yu Wang;Chueh;Yin;Pin;J. Karr;Chi;J. Gunn;C. Loomis;R. Lupton;H. Siddiqui;Shu;Yen;D. Reiley;N. Tamura;Y. Moritani;N. Takato
通讯作者：
N. Takato
斯巴鲁望远镜的主焦点摄谱仪（PFS）：斯巴鲁望远镜的下一代设施仪器已经开始问世
DOI：
10.1117/12.2562206
发表时间：
2020
期刊：
Ground-based and Airborne Instrumentation for Astronomy VIII
影响因子：
--
作者：
N. Tamura;N. Takato;Y. Moritani;K. Yabe;Y. Ishizuka;Y. Kamata;H. Furusawa;J. Greene;J. Gunn;E. Jeschke;S. Kawanomoto;Michitaro Koike;S. Koshida;C. Loomis;S. Mineo;H. Okita;Y. Okura;M. Onodera;J. Rousselle;Kiaina Schubert;H. Siddiqui;D. Spergel;S. Takita;Philip J. Tait;T. Tamura;Masayuki Tanaka;M. Carr;R. Lupton;M. Strauss;Erin Kado;Neven Caplar;R. Ellis;Yoko Tanaka;G. Murray;D. Reiley;Mitsuko K. Roberts;Brent Belland;J. Burnham;M. Seiffert;L. Sodré;Lucio Ramos;M. Takada;H. Murayama;N. Yasuda;Aidan C. Gray;A. Harding;Joshua Peebles;M. Golebiowski;A. Allaoui;S. Arnouts;P. Balard;M. Belhadi;R. Barette;R. Barkhouser;Javier Garciá;P. Chabaud;Hsin;R. C. Chou;Y. Chu;R. Costa;Y. Yamada;T. Yamashita;H. Yoshida;T. Crauchet;Rodrigo P. de Almeida;Antonio Cesar de Oliveira;L. Oliveira;Leandro Henrique dos Santos;K. Dohlen;M. Fabricius;D. Ferreira;R. Hammond;M. Hart;T. Heckman;P. Ho;S. Hope;Shu;Yen;Matthew Wung;Pin;M. Jaquet;J. Karr;M. Kimura;A. Fur;E. Komatsu;V. Lebrun;O. Fèvre;D. L. Mignant;Hung;F. Madec;E. Marguerite;L. Marrara;Dmitry Medvedev;Y. Ohyama;J. Orndorff;S. Pascal;M. Reinecke;J. A. Rosa;Mira Sarkis;A. Schmitt;S. Smee;C. Surace;M. Taghizadeh;A. Thakar;D. Vibert;Chi;Shiang‐Yu Wang;S. Werner;Chih
通讯作者：
Chih