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首页> 外文期刊>Publications of the Astronomical Society of the Pacific >Stabilizing a Fabry-Perot Etalon Peak to 3 cm s(-1) for Spectrograph Calibration
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Stabilizing a Fabry-Perot Etalon Peak to 3 cm s(-1) for Spectrograph Calibration

机译:将Fabry-Perot Etalon峰稳定到3 cm s(-1)以进行光谱仪校准

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摘要

We present a method of frequency stabilizing a broadband etalon that can serve as a high-precision wavelength calibrator for an echelle spectrograph. Using a laser to probe the Doppler-free saturated absorption of the rubidium D-2 line, we stabilize one etalon transmission peak directly to the rubidium frequency. The rubidium transition is an established frequency standard and has been used to lock lasers to fractional stabilities of <10(-12), a level of accuracy far exceeding the demands of radial velocity (RV) searches for exoplanets. The stabilized bandwidth depends on the dispersion characteristics of the etalon. We describe a simple setup designed specifically for use at an observatory and demonstrate that we can stabilize the etalon peak to a relative precision of <10(-10); this is equivalent to 3 cm s(-1) RV precision.
机译:我们提出了一种频率稳定宽带标准具的方法,该方法可以用作阶梯光谱仪的高精度波长校准器。使用激光探测D D-2谱线的无多普勒饱和吸收,我们将一个标准具透射峰直接稳定在to频率上。 transition跃迁是已建立的频率标准,已用于将激光器锁定为小于10(-12)的分数稳定性,其精确度水平远远超过寻找系外行星的径向速度(RV)的要求。稳定的带宽取决于标准具的色散特性。我们描述了一个专门为天文台设计的简单设置,并证明我们可以将标准具的峰值稳定在相对精度<10(-10);这相当于3 cm s(-1)RV精度。

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