MITEoR: A prototype highly scalable interferometer for 21 cm cosmology

J. Dillon, Haoxuan Zheng, Max Tegmark
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Abstract

Studying astrophysics and cosmology with the 21 cm line of neutral hydrogen requires extreme sensitivity and, therefore, radio telescopes with enormous collecting areas. Achieving that size with an interferometer is limited by the computational cost of the correlator, which scales as N2, where N is the number of antennas in the array. However, a large class of highly redundant interferometers can cut that scaling down to N logN. Redundant configurations also enable new algorithms for precise and automated calibration. For this reason we designed MITEoR, a 64-element, dual-polarization prototype radio interferometer designed to demonstrate these scalable technologies, which we constructed at MIT and deployed this summer in The Forks, Maine. We report on the results of MITEoR and the lessons learned for next generation radio interferometers.
MITEoR:用于21厘米宇宙学的高度可扩展干涉仪原型
用21厘米的中性氢线研究天体物理学和宇宙学需要极高的灵敏度,因此需要具有巨大收集区域的射电望远镜。用干涉仪实现这种尺寸受到相关器计算成本的限制,相关器的计算成本为N2,其中N是阵列中天线的数量。然而,大量的高冗余干涉仪可以将这个比例降低到N logN。冗余配置还可以实现精确和自动校准的新算法。出于这个原因,我们设计了MITEoR,一个64单元的双偏振原型无线电干涉仪,旨在展示这些可扩展的技术,我们在麻省理工学院建造并于今年夏天在缅因州的福克斯部署。我们报告MITEoR的结果以及为下一代无线电干涉仪吸取的经验教训。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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