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A fast new cadioptric design for fiber-fed spectrographs

机译:新型快速的光纤馈电光谱仪设计

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The next generation of massively multiplexed multi-object spectrographs (DESpec, SUMIRE, BigBOSS, 4MOST,HECTOR) demand fast, efficient and affordable spectrographs, with higher resolutions (R = 3000-5000) than currentdesigns. Beam-size is a (relatively) free parameter in the design, but the properties of VPH gratings are such that, forfixed resolution and wavelength coverage, the effect on beam-size on overall VPH efficiency is very small. For alltransmissivecameras, this suggests modest beam-sizes (say 80-150mm) to minimize costs; while for cadioptric(Schmidt-type) cameras, much larger beam-sizes (say 250mm+) are preferred to improve image quality and to minimizeobstruction losses. Schmidt designs have benefits in terms of image quality, camera speed and scattered lightperformance, and recent advances such as MRF technology mean that the required aspherics are no longer a prohibitivecost or risk.The main objections to traditional Schmidt designs are the inaccessibility of the detector package, and the loss inthroughput caused by it being in the beam. With expected count rates and current read-noise technology, the gain incamera speed allowed by Schmidt optics largely compensates for the additional obstruction losses. However, futureadvances in readout technology may erase most of this compensation.A new Schmidt/Maksutov-derived design is presented, which differs from previous designs in having the detectorpackage outside the camera, and adjacent to the spectrograph pupil. The telescope pupil already contains a hole at itscenter, because of the obstruction from the telescope top-end. With a 250mm beam, it is possible to largely hide a 6cm ×6cm detector package and its dewar within this hole. This means that the design achieves a very high efficiency,competitive with transmissive designs. The optics are excellent, as least as good as classic Schmidt designs, allowingF/1.25 or even faster cameras. The principal hardware has been costed at $300K per arm, making the design affordable.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:下一代大规模多目标多光谱仪(DESpec,SUMIRE,BigBOSS,4MOST,HECTOR)需要快速,高效和负担得起的光谱仪,其分辨率(R = 3000-5000)比目前的设计更高。光束尺寸在设计中是一个(相对)自由的参数,但是VPH光栅的特性使得在固定的分辨率和波长覆盖范围内,光束尺寸对总体VPH效率的影响非常小。对于所有透射相机,这建议使用适中的光束尺寸(例如80-150mm)以最大程度地降低成本;对于折光(Schmidt型)相机,最好使用更大的光束尺寸(例如250mm +),以提高图像质量并最小化障碍物的损失。施密特(Schmidt)设计在图像质量,相机速度和散射光性能方面具有优势,最近的进步(例如MRF技术)意味着所需的非球面不再是高昂的成本或风险。传统施密特(Schmidt)设计的主要反对意见是无法获得检测器套件,以及由于它在光束中而导致的吞吐量损失。利用预期的计数率和当前的读取噪声技术,施密特光学器件所允许的摄像机内部增益速度在很大程度上弥补了额外的障碍物损失。但是,未来的读数技术进步可能会抵消大部分补偿。提出了一种新的Schmidt / Maksutov衍生的设计,该设计与以前的设计不同之处在于,探测器组件位于相机外部且与光谱仪瞳孔相邻。由于望远镜顶端的阻塞,望远镜瞳孔的中心已经有一个孔。使用250mm的光束,可以将6cm×6cm的检测器包装及其杜瓦瓶大面积隐藏在该孔中。这意味着该设计实现了非常高的效率,与透射型设计相竞争。光学器件非常出色,至少与经典的施密特设计一样好,可以使用F / 1.25甚至更快的摄像头。主要的硬件成本为每支臂30万美元,这使得设计负担得起。©(2012)版权所有,美国光电仪器工程师协会(SPIE)。摘要的下载仅允许个人使用。

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