Collaborative development of next generation instruments

斯巴鲁望远镜的七个常用天文仪器和一个自适应光学系统已经完成。每一台仪器都具有世界顶级的性能和多种功能，它们使斯巴鲁望远镜在天文观测中展示了其高性能。这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 -微弱目标相机和光谱仪-提供光学成像和长缝和多缝光谱超过6弧分的视野。(5)HDS -高色散光谱仪-提供极高分辨率的光谱。(6)IRCS -红外照相机和光谱仪-提供1-5微米的成像，以及相同范围内的低分辨率和中阶梯光谱。(7)OHS/CISCO - OH抑制器/冷却红外光谱仪和OHS相机-提供近红外成像和低分辨率光谱。(8)Suprime-Cam - Subaru Prime Focus Camera -提供了一个大视场的光学成像和一个镶嵌的CCD。此外，还研制了一些用于望远镜性能验证的测试仪器。第二代通用仪器的基本开发，即：e.研制了FMOS -主焦点多目标摄谱仪和MOICS -多目标红外相机和摄谱仪。

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.