探测再电离纪元(PAPER)精密阵列的冗余非成像定标

J. Aguirre, A. Parsons, R. Bradley, C. Carilli, D. DeBoer, Z. Ali, Adrian Liu, D. Jacobs, David F. Moore, J. Pober, I. Stefan
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引用次数: 0

摘要

只提供摘要形式。再电离纪元探测精密阵列(PAPER)是一个旨在探测再电离纪元(EoR)中性氢发射空间功率谱的重点实验。PAPER是一种干涉仪,工作频率为100 - 200兆赫,位于南非未来的平方公里阵列(SKA)站点。PAPER天线测量线性极化,相关器产生全斯托克斯输出。PAPER目前有64个天线,刚刚完成了为期141天的科学整合。扩展到128个天线和另一个长期的观测活动将在2013年底完成。为了达到对功率谱的特定模式的最大灵敏度,PAPER目前采用了高度冗余的阵列配置。这种配置对紫外平面的采样设计非常差,因此不特别适合标准的自校准技术。然而,人们已经知道多年(例如Noordam & de Bruyn 1982),瞬时基线冗余允许一种鲁棒、快速和简单的方法来实现天线之间的相对增益和相位延迟校准。我们考虑了Stokes i的PAPER校准结果的准确性和长期稳定性。仅使用冗余来校准剩余Stokes参数的泄漏项已被证明具有挑战性。我们提出了一种适合于非成像方法的逐基线方法,以获得相对x-y线性偏振延迟并表征剩余泄漏项。我们最后演示了如何将单个基线的相对校准与天空模型的确定解耦,并结合对光谱的可见性进行延迟空间清理(Parsons & Backer 2009),以实现对平滑光谱前景发射的高动态范围抑制。这种方法最大限度地减少了校准误差对最终提高采收率功率谱估计的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Redundant and non-imaging calibration of the Precision Array For Probing The Epoch Of Reionization (PAPER)
Summary form only given. The Precision Array for Probing the Epoch of Reionization (PAPER) is a focused experiment aimed at detecting the spatial power spectrum of neutral hydrogen emission during the Epoch of Reionization (EoR). PAPER is an interferometer operating from 100 - 200 MHz at the site of the future Square Kilometre Array (SKA) site in South Africa. The PAPER antennas measure linear polarization and the correlator produces full-Stokes output. PAPER currently has 64 antennas and has just completed a 141-day science integration. An expansion to 128 antennas and another long observing campaign will be complete in late 2013. In order to achieve maximum sensitivity to particular modes of the power spectrum, PAPER currently employs a highly redundant array configuration. This configuration samples the uv-plane extremely poorly by design, is not therefore particularly suited to standard self-calibration techniques. It has been known for many years (e.g Noordam & de Bruyn 1982), however, that instantaneous baseline redundancy allows a robust, fast and simple method for achieving relative gain and phase delay calibration between antennas. We consider the accuracy and long-term stability of the resulting calibration achieved with PAPER for Stokes I. Calibrating the leakage terms for the remaining Stokes parameters using only redundancy has proved challenging. We present a per-baseline method, appropriate for a non-imaging approach, to obtain the relative x-y linear polarization delay and characterize remaining leakage terms. We finally demonstrate how the decoupling of the individual baselines' relative calibration from the determination of a sky model is used in conjunction with a delay-space CLEANing of the visibility to spectrum (Parsons & Backer 2009) to achieve high-dynamic-range suppression of smooth-spectrum foreground emission. This approach minimizes the effect of calibration errors on the estimation of the final EoR power spectrum.
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