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A High-resolution spectrograph for the 72cm Waltz Telescope at Landessternwarte, Heidelberg

机译:海德堡Landessternwarte的72厘米华尔兹望远镜的高分辨率光谱仪

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摘要

The Waltz Spectrograph is a fiber-fed high-resolution échelle spectrograph for the 72 cm Waltz Telescope at the Landessternwarte, Heidelberg. It uses a 31.6 lines/mm 63.5° blaze angle échelle grating in white-pupil configuration, providing a spectral resolving power of R ~65,000 covering the spectral range between 450-800nm in one CCD exposure. A prism is used for cross-dispersion of échelle orders. The spectrum is focused by a commercial apochromat onto a 2k×2k CCD detector with 13.5μm per pixel. An exposure meter will be used to obtain precise photon-weighted midpoints of observations, which will be used in the computation of the barycentric corrections of measured radial velocities. A stabilized, newly designed iodine cell is employed for measuring radial velocities with high precision. Our goal is to reach a radial velocity precision of better than 5 m/s, providing an instrument with sufficient precision and sensitivity for the discovery of giant exoplanets. Here we describe the design of the Waltz spectrograph and early on-sky results.
机译:华尔兹光谱仪是用于海德堡Landessternwarte的72厘米华尔兹望远镜的光纤馈电高分辨率埃歇尔光谱仪。它在白光瞳配置中使用31.6线/毫米63.5°闪耀角埃谢尔光栅,在一次CCD曝光中提供450〜800nm光谱范围的R〜65,000的光谱分辨能力。棱镜用于埃谢尔订单的交叉分散。通过商用复消色差透镜将光谱聚焦到每像素13.5μm的2k×2k CCD检测器上。曝光计将用于获得精确的光子加权观测中点,该中点将用于计算所测径向速度的重心校正。一种稳定的,新设计的碘池用于高精度测量径向速度。我们的目标是使径向速度精度高于5 m / s,从而为发现大型系外行星提供一种具有足够精度和灵敏度的仪器。在这里,我们描述了华尔兹光谱仪的设计和早期的天空结果。

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