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A new method for correcting fibre barycentre displacements in high resolution spectroscopy

机译:高分辨率光谱中校正光纤重心位移的新方法

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Unpredictable displacements in the photocentre of an optical feed at the entrance slit of a spectrograph producecorresponding barycentre offsets that impose limits to very high resolution schemes. These limitations not only apply todirect light from a science object, but also light relayed via an optical fibre or image slicer. Several mitigation strategiesare in development or are currently in use, however these all have potentially restrictive idiosyncrasies.An alternative approach is proposed to remove displacement effects from the spectra by nulling barycentre offsets.Correction is achieved by time-integrating at the detector a sequence of multiple normal and 180-degree inverted imagesof the input aperture, thus eliminating optical asymmetries about the axis of inversion, which is aligned orthogonal to thespectral direction. The flip is generated with a path-length compensated, non-dispersive ‘reversion prism’, driven on ahigh precision translation stage. The prism is periodically chopped in and out of the beam, and the resulting time-averagedimage thus has an imposed central axis regardless of barycentre shifts.The method works regardless of the specifics of the spectrograph feed (fibre, multiple fibres, slit, slicer etc.) With arelatively simple and inexpensive scheme it should be possible to stabilise an image to better than one part in 10sup4/sup potentially permitting detection down to cmssup-1/sup regimes.The concept is currently at a very early stage of development, so this paper outlines the basic principles and details apractical reversion component that is currently under development at Durham CfAI. There then follows a description ofhow the component will be implemented in a laboratory prototype scheme. The paper concludes with a proposed testplan and suggests the focus for future work.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:在光谱仪的入口狭缝处,光学进给装置的光心的不可预测的位移会产生相应的重心偏移,从而对非常高分辨率的方案施加了限制。这些限制不仅适用于来自科学对象的直接光,而且还适用于通过光纤或图像切片器中继的光。几种缓解策略正在开发中或正在使用中,但是这些策略都有潜在的局限性。一种替代方法是通过使重心偏移为零来消除光谱中的位移效应。垂直和180度反转的输入光圈图像,从而消除了围绕反转轴的光学不对称性,该反转轴与光谱方向正交。翻转是由经过路径长度补偿的非色散“回复棱镜”生成的,并在高精度平移台上驱动。棱镜被周期性地切入和切出光束,因此得到的时间平均图像具有强加的中心轴,而与重心偏移无关。 。)使用相对简单和廉价的方案,应该有可能将图像稳定到优于10 4 的一部分,从而有可能允许检测到cms -1 机制。目前,它还处于开发的早期阶段,因此本文概述了基本原理,并详细介绍了达勒姆CfAI正在开发的实用的复归组件。接下来是关于如何在实验室原型方案中实现该组件的描述。本文以拟议的测试计划作为结束,并提出了未来工作的重点。©(2012)COPYRIGHT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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