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The AEOS spectrograph: Opto-mechanical design and scientific capability.

机译:AEOS光谱仪:光机械设计和科学能力。

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摘要

We have designed, fabricated, and installed a coudé imaging spectrograph for use with the Advanced Electro-Optical System (AEOS) 3.7-meter telescope atop Mt. Haleakala on Maui. The spectrograph is divided into two main subsystems: a visible (∼0.5–01.0 μm) channel and an infrared (∼1.0–2.5 μm) channel, both cross-dispersed echelle spectrometers with resolutions in the 10,000–50,000 range.; Several features have made this endeavor distinctive. The most important was the fact that the AEOS spectrograph was designed to have a spectral resolution sufficiently high enough to clearly resolve the atmospheric OH lines, which are the primary source of background radiation between 0.7–1.8 μm. In the infrared, achieving adequate sensitivity between the OH lines is possible only with the low read noise (5 e rms) and dark current (1 e min−1) of the large-format detectors the HAWAII array development program has demonstrated, thereby making the AEOS spectrograph infrared channel one of the highest resolution astronomical grating spectrometers currently in existence and unique in the science it can accomplish.; The optical design of the spectrographs is based on the “white pupil” concept, where a second collimator allows placing the pupil image on both the echelle and cross-disperser gratings, thus minimizing the size and complexity of the spectrograph camera optics. The white pupil design also allows the echelles to be used very close to true Littrow configuration, thus maximizing grating efficiency.; We present preliminary observations and results obtained with both spectrograph channels. Expected wavelength coverages and dispersions have been achieved. Initial estimates of the visible channel throughput show it to be approximately 6% on average over the wavelength coverage, comparable to the best high-resolution visible echelle spectrometers. The infrared channel requires further testing before accurate throughput and sensitivity characteristics can be derived.; At the time of this work, the slits of the two respective channels are coaligned to within two arcseconds; upcoming installation of an adjustable dichroic will therefore increase the versatility and efficiency of the instrument even further by allowing both visible and infrared spectra to be acquired simultaneously.; The AEOS spectrograph design relied in part upon previous experience at the IfA. Nevertheless, the size and unique features of the infrared spectrograph made its custom design a challenge.
机译:我们已经设计,制造并安装了Coudé成像光谱仪,可与Mt顶部的3.7米的高级电光系统(AEOS)望远镜配合使用。哈雷阿卡拉在毛伊岛。光谱仪分为两个主要子系统:一个可见光通道(〜0.5–01.0μm)和一个红外光通道(〜1.0–2.5μm),这两个交叉色散的埃歇尔光谱仪的分辨率都在10,000–50,000范围内。多项功能使这项工作与众不同。最重要的是,AEOS光谱仪的设计具有足够高的光谱分辨率,可以清晰地分辨大气OH线,这是0.7-1.8μm之间背景辐射的主要来源。在红外线中,只有在低读取噪声(5 e - rms)和暗电流(1 e - min HAWAII阵列开发程序已展示了大型探测器的-1 ,从而使AEOS光谱仪红外通道成为目前最高分辨率的天文光栅光谱仪之一,并且在它可以完成的科学领域中是独一无二的。光谱仪的光学设计基于“白色瞳孔”概念,其中第二个准直仪允许将瞳孔图像放置在阶梯光栅和交叉色散光栅上,从而使光谱仪相机光学器件的尺寸和复杂性最小化。白光瞳孔设计还允许在非常接近真正的Littrow构造的情况下使用切面刀,从而最大程度地提高光栅效率。我们介绍了两种光谱仪通道的初步观测结果。已经实现了预期的波长覆盖范围和色散。可见光通道通过量的初步估计显示,在整个波长范围内,平均可见光通量约为6%,可与最佳高分辨率可见光谱仪相比。红外通道需要进一步测试,才能得出准确的通量和灵敏度特性。在进行这项工作时,两个相应通道的缝隙在两个弧秒内对齐;因此,即将安装的可调二向色镜将通过同时获取可见光谱和红外光谱来进一步提高仪器的多功能性和效率。 AEOS光谱仪的设计部分依赖于IfA的以往经验。然而,红外光谱仪的尺寸和独特功能使其定制设计成为一个挑战。

著录项

  • 作者

    Thornton, Robert J., Jr.;

  • 作者单位

    University of Hawaii.;

  • 授予单位 University of Hawaii.;
  • 学科 Physics Astronomy and Astrophysics.
  • 学位 Ph.D.
  • 年度 2002
  • 页码 153 p.
  • 总页数 153
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天文学;
  • 关键词

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