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THE MANGA INTEGRAL FIELD UNIT FIBER FEED SYSTEM FOR THE SLOAN 2.5 M TELESCOPE

机译:斯隆2.5 M望远镜的MANGA集成现场单纤维进纸系统

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We describe the design, manufacture, and performance of bare-fiber integral field units (IFUs) for the SDSS-IV survey Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) on the the Sloan 2.5 m telescope at Apache Point Observatory. MaNGA is a luminosity-selected integral-field spectroscopic survey of 104 local galaxies covering 360–1030 nm at . The IFUs have hexagonal dense packing of fibers with packing regularity of 3 μm (rms), and throughput of 96 ± 0.5% from 350 nm to 1 μm in the lab. Their sizes range from 19 to 127 fibers (3–7 hexagonal layers) using Polymicro FBP 120:132:150 μm core:clad:buffer fibers to reach a fill fraction of 56%. High throughput (and low focal-ratio degradation (FRD)) is achieved by maintaining the fiber cladding and buffer intact, ensuring excellent surface polish, and applying a multi-layer anti-reflection (AR) coating of the input and output surfaces. In operations on-sky, the IFUs show only an additional 2.3% FRD-related variability in throughput despite repeated mechanical stressing during plate plugging (however other losses are present). The IFUs achieve on-sky throughput 5% above the single-fiber feeds used in SDSS-III/BOSS, attributable to equivalent performance compared to single fibers and additional gains from the AR coating. The manufacturing process is geared toward mass-production of high-multiplex systems. The low-stress process involves a precision ferrule with a hexagonal inner shape designed to lead inserted fibers to settle in a dense hexagonal pattern. The ferrule ID is tapered at progressively shallower angles toward its tip and the final 2 mm are straight and only a few microns larger than necessary to hold the desired number of fibers. Our IFU manufacturing process scales easily to accommodate other fiber sizes and can produce IFUs with substantially larger fiber counts. To assure quality, automated testing in a simple and inexpensive system enables complete characterization of throughput and fiber metrology. Future applications include larger IFUs, higher fill factors with stripped buffer, de-cladding, and lenslet coupling.
机译:我们描述了SDSS-IV勘测在Apache Point天文台Sloan 2.5 m望远镜上的Apache Point天文台(MaNGA)测绘附近星系的裸纤整体场单元(IFU)的设计,制造和性能。 MaNGA是对104个覆盖360–1030 nm的本地星系的光度选择积分场光谱学调查。 IFU在实验室中具有六方密密麻麻的纤维堆积规则,堆积规则为3μm(rms),从350 nm到1μm的吞吐量为96±0.5%。使用Polymicro FBP 120:132:150μm纤芯:包层:缓冲光纤,其尺寸范围从19到127根光纤(3-7六边形层),以达到56%的填充率。通过保持光纤包层和缓冲层完好无损,确保出色的表面抛光并在输入和输出表面上施加多层抗反射(AR)涂层,可以实现高吞吐量(和低焦比降低(FRD))。在空中作业中,尽管在板塞过程中反复受到机械应力(尽管存在其他损失),但IFU在吞吐量方面仅显示出2.3%与FRD相关的额外变化。 IFU可实现SDSS-III / BOSS中使用的单纤维进料的空中生产率高出5%,这归因于与单纤维相比的同等性能以及AR涂层带来的额外收益。制造过程适合大规模生产高多重系统。低应力过程涉及具有六边形内部形状的精密密封垫圈,该形状设计成可将插入的纤维引导成密集的六边形图案。套圈ID朝着其尖端逐渐变浅,逐渐变细,最后2毫米是笔直的,仅比保持所需数量的光纤所需的直径大几微米。我们的IFU制造工艺可以轻松扩展以适应其他尺寸的光纤,并且可以生产出纤维数量大得多的IFU。为了确保质量,在简单且廉价的系统中进行自动测试可以对吞吐量和光纤计量进行全面表征。未来的应用包括更大的IFU,带缓冲层的高填充因子,去覆层和小透镜耦合。
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