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An inexpensive field-widened monolithic Michelson interferometer for precision radial velocity measurements

机译:一种廉价的,宽范围的单片迈克尔逊干涉仪,用于精确的径向速度测量

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We have constructed a thermally compensated field-widened monolithic Michelson interferometer that can be used with a medium-resolution spectrograph to measure precise Doppler radial velocities of stars. Our prototype monolithic fixed-delay interferometer is constructed with off-the-shelf components and assembled using a hydrolysis bonding technique. We installed and tested this interferometer in the Exoplanet Tracker (ET) instrument at the Kitt Peak 2.1 m telescope, an instrument built to demonstrate the principles of dispersed fixed-delay interferometry. An iodine cell allows the interferometer drift to be accurately calibrated, relaxing the stability requirements on the interferometer itself. When using our monolithic interferometer, the ET instrument has no moving parts (except the iodine cell), greatly simplifying its operation. We demonstrate differential radial velocity precision of a few ms(-1) on well known radial velocity standards and planet bearing stars when using this interferometer. Such monolithic interferometers will make it possible to build relatively inexpensive instruments that are easy to operate and capable of precision radial velocity measurements. A larger multiobject version of the Exoplanet Tracker will be used to conduct a large scale survey for planetary systems as part of the Sloan Digital Sky Survey III (SDSS III). Variants of the techniques and principles discussed in this paper can be directly applied to build large monolithic interferometers for such applications, enabling the construction of instruments capable of efficiently observing many stars simultaneously at high velocity precision.
机译:我们构建了一个热补偿的场宽单片迈克尔逊干涉仪,该干涉仪可以与中分辨率光谱仪一起使用,以测量恒星的精确多普勒径向速度。我们的原型单片固定延迟干涉仪由现成的组件构成,并使用水解键合技术进行组装。我们在Kitt Peak 2.1 m望远镜的Exoplanet Tracker(ET)仪器中安装并测试了该干涉仪,该仪器旨在证明分散固定延迟干涉仪的原理。碘池可精确校准干涉仪的漂移,从而减轻了干涉仪本身的稳定性要求。当使用我们的整体式干涉仪时,ET仪器没有活动部件(碘池除外),从而大大简化了操作。当使用这种干涉仪时,我们证明了在众所周知的径向速度标准和行星轴承恒星上几ms(-1)的微分径向速度精度。这种整体式干涉仪将使得有可能制造相对便宜的仪器,该仪器易于操作并且能够进行精确的径向速度测量。作为Sloan Digital Sky Survey III(SDSS III)的一部分,将使用更大的多物体版本的系外行星追踪器进行行星系统的大规模测量。本文讨论的技术和原理的各种变体可以直接应用于构建用于此类应用的大型单片干涉仪,从而能够构建能够以高速度精度同时有效观测许多恒星的仪器。

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