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arXiv 2311.03494astro-ph.IMastro-ph.CO
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局地环境对紧凑型射电干涉仪的影响 I:天籁碟形探路者阵列中的交叉耦合

The Effects of the Local Environment on a Compact Radio Interferometer I: Cross-coupling in the Tianlai Dish Pathfinder Array

Juhun Kwak, John Podczerwinski, Peter Timbie, Réza Ansari, John Marriner, Albert Stebbins, Fengquan Wu, Haotian Cao, Xuelei Chen, Kai He, Jixia Li, Shijie Sun, Jiacong Zhu

AI总结:

本研究针对紧凑型射电干涉仪受局地环境产生的非天文相关信号干扰的问题,建立天线接收机噪声交叉耦合模型,应用于天籁碟形探路者阵列并结合观测验证,提出21 cm强度测绘仪器的交叉耦合水平要求。

摘要:

射电天文干涉仪测量的可见度包含由阵列局地环境产生的非天文相关信号。这类相关信号在专为21 cm强度测绘研发的紧凑型阵列中影响尤为显著,受污染的可见度幅度可能超过预期的21 cm信号,构成重要的系统误差。我们研究了紧凑型阵列中天线辐射的接收机噪声,并建立了其与其他天线耦合方式的模型。我们将该模型应用于天籁碟形探路者阵列(TDPA)——一个由16面6米碟形天线组成的紧凑型阵列。耦合模型结合了电磁仿真、网络分析仪测量以及接收机噪声测量。我们将模型结果与阵列的漂移扫描观测结果进行对比,并提出了21 cm强度测绘仪器所需的天线交叉耦合水平要求。研究发现,对于TDPA而言,交叉耦合必须降低待定(TBD)个数量级,才能使其对可见度的影响可忽略不计。

英文摘要:

The visibilities measured by radio astronomical interferometers include non-astronomical correlated signals that arise from the local environment of the array. These correlated signals are especially important in compact arrays such as those under development for 21\,cm intensity mapping. The amplitudes of the contaminated visibilities can exceed the expected 21\,cm signal and represent a significant systematic effect. We study the receiver noise radiated by antennas in compact arrays and develop a model for how it couples to other antennas. We apply the model to the Tianlai Dish Pathfinder Array (TDPA), a compact array of 16, 6-m dish antennas. The coupling model includes electromagnetic simulations, measurements with a network analyzer, and measurements of the noise of the receivers. We compare the model to drift-scan observations with the array and set requirements on the level of antenna cross-coupling for 21\,cm intensity mapping instruments. We find that for the TDPA, cross-coupling would have to be reduced by TBD orders of magnitude in order to contribute negligibly to the visibilities.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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