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Development of a near-infrared wide-field integral field unit by ultra-precision diamond cutting
Journal of Astronomical Telescopes, Instruments, and Systems ( IF 1.7 ) Pub Date : 2024-03-01 , DOI: 10.1117/1.jatis.10.1.015004 Kosuke Kushibiki 1 , Shinobu Ozaki 2 , Masahiro Takeda 3 , Takuya Hosobata 3 , Yutaka Yamagata 3 , Shinya Morita 4 , Toshihiro Tsuzuki 2 , Keiichi Nakagawa 5 , Takao Saiki 6 , Yutaka Ohtake 6 , Kenji Mitsui 2 , Hirofumi Okita 7 , Yutaro Kitagawa 1 , Yukihiro Kono 1 , Kentaro Motohara 2 , Hidenori Takahashi 8 , Masahiro Konishi 1 , Natsuko Kato 1 , Shuhei Koyama 1 , Nuo Chen 2
Journal of Astronomical Telescopes, Instruments, and Systems ( IF 1.7 ) Pub Date : 2024-03-01 , DOI: 10.1117/1.jatis.10.1.015004 Kosuke Kushibiki 1 , Shinobu Ozaki 2 , Masahiro Takeda 3 , Takuya Hosobata 3 , Yutaka Yamagata 3 , Shinya Morita 4 , Toshihiro Tsuzuki 2 , Keiichi Nakagawa 5 , Takao Saiki 6 , Yutaka Ohtake 6 , Kenji Mitsui 2 , Hirofumi Okita 7 , Yutaro Kitagawa 1 , Yukihiro Kono 1 , Kentaro Motohara 2 , Hidenori Takahashi 8 , Masahiro Konishi 1 , Natsuko Kato 1 , Shuhei Koyama 1 , Nuo Chen 2
Affiliation
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.
中文翻译:
超精密金刚石切割近红外宽视场整体视场单元研制
积分场光谱 (IFS) 是一种在单次曝光中获得特定视场 (FoV) 空间分辨光谱的观测方法。近年来,近红外 IFS 在观测具有强尘埃衰减或高红移的物体方面变得越来越重要。与光学仪器相比,现有近红外 IFS 仪器的局限性之一是其 FoV 相对较小,小于 100 arcsec2。因此,我们通过将切片宽度与0.4角秒的典型视宁尺寸相匹配,开发了一种近红外(0.9至2.5μm)图像切片器型积分场单元(IFU),其FoV为13.5×10.4角秒2。IFU 具有紧凑的光学设计,利用离轴椭球面镜来减少像差。使用超精密切割机制造复杂的光学元件,表面粗糙度均方根小于 10 nm,PV 形状误差小于 300 nm。超精密加工还可以简化对准程序。空中性能评估证实了 IFU 的图像质量和吞吐量符合设计。总之,我们利用超精密切割技术成功开发了紧凑型IFU,几乎满足要求。
更新日期:2024-03-04
中文翻译:
超精密金刚石切割近红外宽视场整体视场单元研制
积分场光谱 (IFS) 是一种在单次曝光中获得特定视场 (FoV) 空间分辨光谱的观测方法。近年来,近红外 IFS 在观测具有强尘埃衰减或高红移的物体方面变得越来越重要。与光学仪器相比,现有近红外 IFS 仪器的局限性之一是其 FoV 相对较小,小于 100 arcsec2。因此,我们通过将切片宽度与0.4角秒的典型视宁尺寸相匹配,开发了一种近红外(0.9至2.5μm)图像切片器型积分场单元(IFU),其FoV为13.5×10.4角秒2。IFU 具有紧凑的光学设计,利用离轴椭球面镜来减少像差。使用超精密切割机制造复杂的光学元件,表面粗糙度均方根小于 10 nm,PV 形状误差小于 300 nm。超精密加工还可以简化对准程序。空中性能评估证实了 IFU 的图像质量和吞吐量符合设计。总之,我们利用超精密切割技术成功开发了紧凑型IFU,几乎满足要求。