Development of a near-infrared wide-field integral field unit by ultra-precision diamond cutting

IF 1.7 3区 工程技术 Q2 ENGINEERING, AEROSPACE Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-03-01 DOI:10.1117/1.jatis.10.1.015004
Kosuke Kushibiki, Shinobu Ozaki, Masahiro Takeda, Takuya Hosobata, Yutaka Yamagata, Shinya Morita, Toshihiro Tsuzuki, Keiichi Nakagawa, Takao Saiki, Yutaka Ohtake, Kenji Mitsui, Hirofumi Okita, Yutaro Kitagawa, Yukihiro Kono, Kentaro Motohara, Hidenori Takahashi, Masahiro Konishi, Natsuko Kato, Shuhei Koyama, Nuo Chen
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Abstract

Integral field spectroscopy (IFS) is an observational method for obtaining spatially resolved spectra over a specific field of view (FoV) in a single exposure. In recent years, near-infrared IFS has gained importance in observing objects with strong dust attenuation or at a high redshift. One limitation of existing near-infrared IFS instruments is their relatively small FoV, less than 100 arcsec2, compared with optical instruments. Therefore, we developed a near-infrared (0.9 to 2.5 μm) image-slicer type integral field unit (IFU) with a larger FoV of 13.5×10.4 arcsec2 by matching a slice width to a typical seeing size of 0.4 arcsec. The IFU has a compact optical design utilizing off-axis ellipsoidal mirrors to reduce aberrations. Complex optical elements were fabricated using an ultra-precision cutting machine to achieve root mean square surface roughness of less than 10 nm and a P-V shape error of less than 300 nm. The ultra-precision machining can also simplify the alignment procedures. The on-sky performance evaluation confirmed that the image quality and the throughput of the IFU were as designed. In conclusion, we successfully developed a compact IFU utilizing an ultra-precision cutting technique, almost fulfilling the requirements.
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利用超精密钻石切割技术开发近红外宽视场积分场装置
积分场光谱学(IFS)是一种通过一次曝光获得特定视场(FoV)空间分辨率光谱的观测方法。近年来,近红外积分场光谱在观测尘埃衰减较强或红移较高的天体方面越来越重要。与光学仪器相比,现有的近红外 IFS 仪器的一个局限性是视场相对较小,不足 100 弧秒2。因此,我们开发了一种近红外(0.9 至 2.5 μm)图像切片积分场装置(IFU),通过将切片宽度与 0.4 弧秒的典型视场大小相匹配,使其具有 13.5×10.4 弧秒2 的更大视场。IFU 采用紧凑的光学设计,利用离轴椭圆镜减少像差。复杂的光学元件是用超精密切割机制造的,以实现均方根表面粗糙度小于 10 nm,P-V 形误差小于 300 nm。超精密加工还能简化校准程序。天空性能评估证实,IFU 的图像质量和吞吐量均符合设计要求。总之,我们利用超精密切割技术成功研制出了紧凑型 IFU,基本满足了要求。
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来源期刊
CiteScore
4.40
自引率
13.00%
发文量
119
期刊介绍: The Journal of Astronomical Telescopes, Instruments, and Systems publishes peer-reviewed papers reporting on original research in the development, testing, and application of telescopes, instrumentation, techniques, and systems for ground- and space-based astronomy.
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