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SMART Precision Interferometry at 794 nm

机译:794 nm的SMART精密干涉仪

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Single-mode fibers have been used in the near-infrared to dramatically reduce calibration error for long-baseline interferometry. We have begun an effort to apply the advantages of spatial filtering at visible wavelengths for precision measurements of pulsating Cepheids using the IOTA interferometer. Rather than employing photometric taps to calibrate fluctuating coupling efficiency, we are using an "asymmetric" coupler which allows this calibration to be done without losing photons. The Single-Mode Asymmetric Recombination Technique (SMART) experiment has finished lab-testing, and has been installed at IOTA for full commissioning in Summer 2002. We report the results of lab characterization and first sky tests, as well as first fringes on a star using a visible-wavelength single-mode coupler. With both lab and sky experience using unpolarized light, we have found that circular silica fibers are quite practical for precision interferometric measurements. We conclude that circular fibers (as opposed to polarization maintaining fibers) have an undeserved poor reputation and that birefringence effects pose no significant difficulty.
机译:在近红外中已使用单模光纤,以大大降低长基线干涉测量法的校准误差。我们已开始努力利用可见光波长处的空间滤波优势,利用IOTA干涉仪精确测量脉动造父变星。我们没有使用光度学抽头来校准波动的耦合效率,而是使用“非对称”耦合器,该耦合器可以在不损失光子的情况下完成该校准。单模不对称复合技术(SMART)实验已完成实验室测试,并已安装在IOTA上,并于2002年夏季进行全面调试。我们报告了实验室表征和首次星空测试以及恒星上第一条纹的结果使用可见波长单模耦合器。凭借在实验室和天空中使用非偏振光的经验,我们发现圆形二氧化硅光纤对于精密干涉测量非常实用。我们得出的结论是,圆形光纤(与保偏光纤相反)声誉不佳,并且双折射效应不会带来很大的困难。

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