曼弗雷德·赫斯行星摄谱仪实现了环境稳定性

Vanessa Fahrenschon, H. Kellermann, Liang Wang, F. Grupp, C. Goessl, U. Hopp, W. Mitsch, M. Schmidt, C. Ries, J. Steuer, R. Saglia, R. Bender
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引用次数: 1

摘要

曼弗雷德·希尔特行星摄谱仪(MaHPS)——以前也被称为FOCES——是位于温德尔斯坦天文台2米望远镜上的高分辨率梯队摄谱仪。它的主要科学目标之一是探测几米/秒级别的行星。为了在长期范围内实现如此高的精度,需要仪器的环境稳定性。介绍了目前使用的温度和压力控制系统,并提出了两种不同的温度控制设置,分别有两个和三个主动控制层。用天文频率梳(AFC)作为校准器进行了一系列测量,以说明系统的性能。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Environmental stability achieved for the Manfred Hirth Planet Spectrograph
The Manfred Hirt Planet Spectrograph (MaHPS) — formerly also referred to as FOCES — is a high-resolution echelle spectrograph at the 2m telescope of the Wendelstein Observatory. One of its main scientific goals is the detection of planets at the few m/s level. To achieve such high precisions on a long-term scale, environmental stabilization of the instrument is required. The currently used temperature and pressure control systems are introduced and we present two different temperature control setups, with two and three actively controlled layers respectively. A series of measurements with an Astro Frequency Comb (AFC) as calibrator is shown to illustrate the system performance.
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