Collaborative development of next generation instruments

下一代仪器的协作开发

• 批准号: 11694107
• 负责人: KAIFU Norio
• 金额: $ 17.92万
• 依托单位: National Astronomical Observatory
• 依托单位国家: 日本
• 项目类别: Grant-in-Aid for Scientific Research (A)
• 财政年份: 1999
• 资助国家: 日本
• 起止时间: 1999 至 2000
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-11694107/
• 关键词: astronomy; optical and infrared astronomy; astronomical telescecop; astronomical instruments; instrumentation; observation system; 天文データ解析システム; 大望遠鏡; 観測装置; 制御システム

Seven common-use astronomical instruments and one adaptive optics system for the Subaru telescope have been completed. Each of the instruments has a world top-level performance and many functions and they allow the Subaru telescope to demonstrate its high performance in astronomical observation. The seven instruments and the adaptive optics system are the follows : (1) AO - Subaru Adaptive Optics system - delivers diffraction-limited images in the near infrared. (2) CIAO - Coronagraphic Imager with Adaptive Optics - provides a near-infrared imaging capability in the vicinity of bright sources. (3) COMICS - Cooled Mid-Infrared Camera and Spectrograph - provides imaging and spectroscopy from 8-20 microns. (4) FOGAS - Faint Object Camera And Spectrograph - provides optical imaging and longslit and multi-slit spectroscopy over a 6 arcmin field of view. (5) HDS - High Dispersion Spectrograph - provides extremely high-resolution optical spectroscopy. (6) IRCS - Infrared Camera and Spectrograph - provides imaging from 1-5 microns, and low resolution and echelle spectroscopy over the same range. (7) OHS/CISCO - OH Suppressor/Cooled Infrared Spectrograph and Camera for OHS - provides imaging and low-resolution spectroscopy in the near-infrared. (8) Suprime-Cam - Subaru Prime Focus Camera - provides optical imaging over a large field of view with a mosaic ofCCDs. In addition, some test instruments for performance verification of the telescope were developed. Fundamental development for the second-generation common-use instruments, i. e. FMOS - prime-focus multi object Spectrograph, and MOICS - multi object infrared camera and Spectrograph, were also made.

7台常用天文仪器和1台斯巴鲁望远镜自适应光学系统已经完成。每台仪器都具有世界顶级的性能和众多的功能，使斯巴鲁望远镜在天文观测中展示了它的高性能。七个仪器和自适应光学系统如下：(1)AO -斯巴鲁自适应光学系统-提供近红外衍射限制图像。(2) CIAO -具有自适应光学的日冕成像仪-在明亮光源附近提供近红外成像能力。(3) COMICS -冷却中红外相机和光谱仪-提供8-20微米的成像和光谱。(4) FOGAS -微弱物体相机和摄谱仪-提供光学成像和长缝和多缝光谱在6角分视场。(5) HDS -高色散光谱仪-提供极高分辨率的光学光谱。(6) IRCS -红外相机和光谱仪-提供1-5微米的成像，以及相同范围内的低分辨率和梯队光谱。(7) OHS/CISCO - OH抑制器/ OHS冷却红外光谱仪和相机-提供近红外成像和低分辨率光谱。(8) Prime - cam -斯巴鲁Prime - Focus相机-提供光学成像在一个大的视场与马赛克的ccd。此外，还研制了一些用于望远镜性能验证的测试仪器。第二代通用仪器，即FMOS -定焦多目标摄谱仪和MOICS -多目标红外摄像机和摄谱仪也取得了基础性的发展。

项目成果

KENTARO MOTOHARA: "Infrared Imaging of z=2.43 Radio Galaxy B3 0731 + 438 with the Subaru Telescope - Detection of H α Ionization Cones of a Powerful Radio Galaxy"Publications of the Astronomical Society of Japan. 52巻1号. 33-41 (2000)

KENTARO MOTOHARA：“使用 Subaru 望远镜对 z=2.43 射电星系 B3 0731 + 438 进行红外成像 - 检测强大射电星系的 H α 电离锥”日本天文学会出版物第 52 卷第 1. 33 期。 41 (2000)

Kaifu, Norio, et al.: "The First Light of the Subaru Telescope : A New Infrared Image of the Orion Nebula"Publications of the Astronomical Society of Japan. 52. 1-8 (2000)

Kaifu、Norio 等人：“斯巴鲁望远镜的第一束光：猎户座星云的新红外图像”日本天文学会出版物。

FUMIHIDE IWAMURO: "Imfrared Imaging of the Gravitational Lens PG 1115+080 with the Subaru Telescope"Publications of the Astronomical Society of Japan. 52巻1号. 25-32 (2000)

FUMIHIDE IWAMURO：“使用 Subaru 望远镜对引力透镜 PG 1115+080 进行红外成像”，日本天文学会出版物，第 52 卷，第 1. 25-32 期（2000 年）。

Iye, Masanori, et al.: "Subaru First-Light Deep Photometry of Galaxies in A 851 Field"Publications of the Astronomical Society of Japan. 52. 9-24 (2000)

Iye, Masanori, et al.：“Subaru First-Light Deep Photometry of Galaxies in A 851 Field”日本天文学会出版物。

Kajisawa, Masaru, et al.: "Subaru Observations for the K-Band Luminosity Distribution of Galaxies in Clusters near to 3C 324 at z〜1.2"Publications of the Astronomical Society of Japan. 52. 63-60 (2000)

Kajisawa, Masaru, et al.: “Subaru Observations for the K-Band Luminosity Distribution of Galaxies in close to 3C 324 at z~1.2” 日本天文学会出版物 52. 63-60 (2000)。