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An Inexpensive Field-Widened Monolithic Michelson Interferometer for Precision Radial Velocity Measurements

机译:一种廉价的现场拓扑单片迈克尔逊干涉仪   精密径向速度测量

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摘要

We have constructed a thermally compensated field-widened monolithicMichelson interferometer that can be used with a medium-resolution spectrographto measure precise Doppler radial velocities of stars. Our prototype monolithicfixed-delay interferometer is constructed with off-the-shelf components andassembled using a hydrolysis bonding technique. We installed and tested thisinterferometer in the Exoplanet Tracker (ET) instrument at the Kitt Peak 2.1mtelescope, an instrument built to demonstrate the principles of dispersed fixeddelay interferometry. An iodine cell allows the interferometer drift to beaccurately calibrated, relaxing the stability requirements on theinterferometer itself. When using our monolithic interferometer, the ETinstrument has no moving parts (except the iodine cell), greatly simplifyingits operation. We demonstrate differential radial velocity precision of a few ms$^{-1}$ on well known radial velocity standards and planet bearing stars whenusing this interferometer. Such monolithic interferometers will make itpossible to build relatively inexpensive instruments that are easy to operateand capable of precision radial velocity measurements. A larger multi-objectversion of the Exoplanet Tracker will be used to conduct a large scale surveyfor planetary systems as part of the Sloan Digital Sky Survey III (SDSS III).Variants of the techniques and principles discussed in this paper can bedirectly applied to build large monolithic interferometers for suchapplications, enabling the construction of instruments capable of efficientlyobserving many stars simultaneously at high velocity-precision.
机译:我们构建了一个热补偿的场宽单片米歇尔森干涉仪,该干涉仪可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,该仪器旨在演示分散固定延迟干涉测量法的原理。碘池可以对干涉仪的漂移进行精确校准,从而放宽了对干涉仪本身的稳定性要求。当使用我们的单片干涉仪时,ETinstrument没有活动部件(碘池除外),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,几毫秒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,将使用更大的多目标系外行星追踪器对行星系统进行大规模测量。本文讨论的各种技术和原理可以直接应用于构建大型系统。用于此类应用的单片干涉仪,使得能够构建能够以高精度同时高效观测许多恒星的仪器。

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