首页> 外文会议>Conference on ground-based and airborne instrumentation for astronomy IV >Investigating spectrograph design parameters with the Yale Doppler diagnostic facility
【24h】

Investigating spectrograph design parameters with the Yale Doppler diagnostic facility

机译:使用Yale Doppler诊断工具调查光谱仪设计参数

获取原文

摘要

The detection of earth-like exoplanets with the Doppler technique requires extreme precision spectrographs stable overtimescales of years. The precision requirement of 10 cm/s is equivalent to a relative uncertainty of 3x10sup-10/sup, and, with the typical dispersion of the Echelle spectrographs used for this purpose, translates to a shift of a few nanometers of the spectrum on the detector. Consequently, the instrument must be well understood and optimized in every component and detail. We describe the Yale Doppler diagnostic facility (YDDF), a dedicated bench mounted Echelle spectrograph inour lab at Yale University, which will be used to systematically study the influence of different components at thisprecision level. The spectrograph bench allows for a flexible optical configuration, high resolution and sampling, andwide spectral coverage. Further, we incorporated a turbulence and guiding simulator to realistically reproduce thesituation at the telescope, enabling end-to-end tests of important parameters.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:用多普勒技术探测类似地球的系外行星需要极高精密度的光谱仪,需要稳定多年的时间。 10 cm / s的精度要求等效于3x10 -10 的相对不确定度,并且为此目的使用的Echelle光谱仪的典型色散会转化为几纳米的位移。检测器上的光谱。因此,必须在每个组件和细节上充分理解和优化该仪器。我们描述了耶鲁大学多普勒诊断设备(YDDF),这是耶鲁大学专用的台式Echelle光谱仪实验室,将用于在此精度级别上系统地研究不同组件的影响。光谱台可实现灵活的光学配置,高分辨率和采样以及宽光谱范围。此外,我们并入了湍流和引导模拟器,以在望远镜上真实再现场景,从而实现了重要参数的端到端测试。©(2012)COPYRIGHT光电仪器工程师协会(SPIE)。摘要的下载仅允许个人使用。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号