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A new photolithography based technique to mass produce microlens+fibre based integralfield units (IFUs) for 2D spectroscopy

机译:一种新的基于光刻的技术,可大量生产基于微透镜+光纤的积分场单元(IFU),用于二维光谱

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Long-slit astronomical spectroscopy has various limitations when dealing with optimum slit width, atmospheric dispersion, extended source spectroscopy, etc. to name a few. Most of these issues can be solved by the use of optical fibers as the light carrier from the telescope focal plane to the spectrograph. The approach is technically and scientifically flexible in terms of instrument modularity and target acquisition. Implementation of Integral Field Unit (IFU) provides a continuous sampling of extended objects and has a distinct advantage over the single fiber. Using a microlens array in front of the fibers improves the sky coverage by increasing the fill factor. Dev-asthal Optical Telescope Integral Field Spectrograph (DOTIFS) is a novel instrument being built by the Inter-University Centre for Astronomy & Astrophysics, Pune for the 3.6m Devasthal Optical Telescope (DOT) constructed by Aryabhatta Research Institute of Observational Sciences, Nainital. Each of the 16 DOTIFS IFUs consist of 12×12 spatial elements (spaxels) distributed in a hexagonal honeycomb structure covering 8.7"×7.8" in the sky. Each IFU is made by a photolithography technique to transfer the corresponding microlens array pattern to create a mask which holds the fibers at the focal plane end of an integral field unit. These masks are aligned with the microlens array and fibers are inserted before gluing and polishing. The fiber array can be positioned with a peak positioning error less than 5 μm from the desired position within a fiber array, compared to a requirement of 10 μm. The slit end is made by wire EDM cutting technology and fibers are placed with an accuracy of ~0.3 pixels compared to a 6.75 pixel center-to-center gap between two spectra on the detector. In this paper we provide details of deriving requirements and error budgets. The process of photolithography and the use of generated masks to create an IFU are also discussed. The technique allows very cost effective mass production of IFUs which are very accurately matched with the corresponding microlens array.
机译:长缝天文光谱学在处理最佳缝隙宽度,大气色散,扩展源光谱学等方面有多种局限性。这些问题中的大多数可以通过使用光纤作为从望远镜焦平面到光谱仪的光载体来解决。在仪器模块化和目标获取方面,该方法在技术和科学上都非常灵活。整体现场单元(IFU)的实施提供了扩展对象的连续采样,并且比单根光纤具有明显的优势。在光纤前面使用微透镜阵列可通过增加填充系数来改善天空覆盖率。 Dev-asthal光学望远镜积分场光谱仪(DOTIFS)是由大学国际天文与天体物理学中心(Pune)合作为奈奈塔尔Aryabhatta观察科学研究所建造的3.6m Devasthal光学望远镜(DOT)研制的新型仪器。 16个DOTIFS IFU中的每一个都由12×12个空间元素(Spaxels)组成,这些空间元素分布在六边形蜂窝结构中,在天空中覆盖8.7英寸×7.8英寸。每个IFU通过光刻技术制成,以转移相应的微透镜阵列图案,以创建一个将光纤固定在积分场单元的焦平面端的掩模。这些掩模与微透镜阵列对齐,并在粘合和抛光之前插入光纤。相比于10μm的要求,可以以距纤维阵列内所需位置小于5μm的峰值定位误差来定位纤维阵列。狭缝末端是通过线切割加工技术制造的,光纤的放置精度约为0.3像素,而检测器上两个光谱之间的中心距为6.75像素。在本文中,我们提供了派生要求和错误预算的详细信息。还讨论了光刻工艺以及使用生成的掩模创建IFU的过程。该技术允许非常经济高效地批量生产IFU,该IFU与相应的微透镜阵列非常精确地匹配。

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