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Fiber scrambling for precise radial velocities at Lick and Keck Observatories

机译:里克和凯克天文台进行光纤加扰以实现精确的径向速度

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The detection of Earth analogs with radial velocity requires extreme Doppler precision and long term stability.Variations in the illumination of the slit and of the spectrograph optics occur on time scales of seconds andminutes, primarily because of guiding, seeing and focusing. These variations yield differences in the instrumentalprofile (IP). In order to stabilize the IP, we designed a fiber feed for the Hamilton spectrograph at Lick and forHIRES at Keck. Here, we report all results obtained with these fiber scramblers. We also present the design ofa new double scrambler/pupil slicer for HIRES at Keck.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:检测具有径向速度的地球类似物需要极高的多普勒精度和长期稳定性。狭缝和光谱仪光学器件的照明变化在几秒钟和几分钟的时间内就会发生,这主要是由于引导,观察和聚焦。这些变化会产生乐器轮廓(IP)的差异。为了稳定IP,我们为Lick的Hamilton光谱仪和Keck的forHIRES设计了一种光纤馈线。在这里,我们报告使用这些光纤加扰器获得的所有结果。我们还在Keck展示了一种用于HIRES的新型双加扰器/瞳孔切片机的设计。©(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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