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The Habitable-zone Planet Finder: A status update on the development of a stabilized fiber-fed near-infrared spectrograph for the Hobby-Eberly telescope

机译:宜居区行星搜寻器:用于Hobby-Eberly望远镜的稳定光纤馈入近红外光谱仪开发的最新状态

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The Habitable-Zone Planet Finder is a stabilized, fiber-fed, NIR spectrograph being built for the 10m Hobby-Eberly telescope (HET) that will be capable of discovering low mass planets around M dwarfs. The optical design of the HPF is a white pupil spectrograph layout in a vacuum cryostat cooled to 180 K. The spectrograph uses gold-coated mirrors, a mosaic echelle grating, and a single Teledyne Hawaii-2RG (H2RG) NIR detector with a 1.7-micron cutoff covering parts of the information rich z, Y and J NIR bands at a spectral resolution of R~50,000. The unique design of the HET requires attention to both near and far-field fiber scrambling, which we accomplish with double scramblers and octagonal fibers. In this paper we discuss and summarize the main requirements and challenges of precision RV measurements in the NIR with HPF and how we are overcoming these issues with technology, hardware and algorithm developments to achieve high RV precision and address stellar activity.
机译:可居住区行星搜寻器是为10m的Hobby-Eberly望远镜(HET)制作的,稳定的,纤维喂食的NIR光谱仪,它将能够发现M矮星周围的低质量行星。 HPF的光学设计是在冷却至180 K的真空低温恒温器中的白色瞳孔光谱仪布局。该光谱仪使用镀金镜面,镶嵌埃切尔光栅和单个带1.7-R的Teledyne Hawaii-2RG(H2RG)NIR检测器。微米截止值涵盖了信息丰富的z,Y和J NIR波段的部分,光谱分辨率为R〜50,000。 HET的独特设计要求同时关注近场和远场光纤加扰,这是我们使用双加扰器和八边形光纤完成的。在本文中,我们讨论并总结了使用HPF在NIR中进行精确RV测量的主要要求和挑战,以及我们如何通过技术,硬件和算法开发来克服这些问题,以实现较高的RV精度并解决恒星活动。

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