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Optical design of the highly cost optimized new Hector Spectrograph

机译:光学设计高度成本优化的新赫克托克光谱仪

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Hector is a multi-IFU spectrograph in phase-A building for the Anglo-Australian Telescope (AAT) using fibers. Its goal is to observe 30,000 galaxies when fully complete. It is a follow up instrument of SAMI which has 13 IFUs 15" wide. The full project will have a 2 degree field corrector and at least 3 spectrographs. The IFUs are hexabundles 15" to 30" wide made of bare fibers with no buffer tightly packed and fused together to minimize the surface losses between their cores. Many different transparent spectrograph designs were studied covering a large parameter space. An important trade-off study was between the use of microlenses on the slit or just bare fibers. Microlenses have disadvantages but permit considerable simplification of the collimator by making the beam very slow. With microlenses, the collimator can be a unique spherical plano-convex lens significantly smaller than the mirror that would be needed in a reflective design. In the first part of the design, 26 different cameras where designed to cover the parameter space for 2k x 2k, 2k x 4k, or 4k x 4k detectors, and for 50, 75 or 100 micron fiber cores, with or without microlenses, with a triplet in the camera or a doublet plus singlet, and with a maximum wavelength of 1 or 1.05 microns. Not all combinations were designed but for each parameter there are at least two representative cameras with all other parameters identical. A preliminary cost estimate was made for the most promising designs which permitted to reduce them to 3 set of parameters for detailed designing, then to 2 with 4k x 4k detectors and 100 micron fiber cores. One design was made to be simple and low risk with only singlets in the collimator and cameras, the other complex with a mirror in the collimator, doublets and triplets, and innovations that could give better performance at a lower cost but with increased risk. For similar cost, the safe design has lower performances but also lower risks than the complex design. In the final st
机译:Hector是一种使用纤维的Anglo-Australian望远镜(AAT)的阶段建筑物的多IFU光谱仪。它的目标是在完全完成时观察30,000个星系。它是萨米的后续仪器,其中有13 IFUS 15“宽。完整的项目将具有2度的场地校正器和至少3个光谱仪。IFUS是由裸纤维制成的15”到30“宽,没有缓冲纤维包装并融合在一起以最小化其核心之间的表面损失。研究了许多不同的透明光谱仪设计,覆盖了一个大的参数空间。重要的权衡研究是在狭缝或只是裸纤维上使用微透镜。微透镜有缺点但是通过使光束非常慢,可以大大简化准直器。使用微透镜,准直器可以是独特的球形平面凸透镜,明显小于反射设计中所需的镜子。在设计的第一部分,26不同的相机,其中设计用于覆盖2k x 2k,2k x 4k或4k x 4k探测器的参数空间,以及50,75或100微米纤维芯,有或没有微透镜相机或双峰加单线片中的三联网,最大波长为1或1.05微米。并非所有组合都被设计,但对于每个参数,至少有两个具有相同其他参数的代表性相机。初步成本估算是对最有前途的设计进行了估算,允许将它们减少到3组参数以进行详细设计,然后使用4K x 4K检测器和100微米纤维芯。一种设计是简单而低的风险,只有准直器和摄像机中的单体,另一个复合物,在准直器,双峰和三胞胎中的镜子,以及可以以更低的成本提供更好的性能但具有增加的风险。出于类似的成本,安全设计具有较低的性能,但较低的风险是比复杂的设计更低。在最后的st

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