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BAORadio: A digital pipeline for radio interferometry and 21 cm mapping of large scale structures

机译:BAORadio:用于无线电干涉测量和大型结构的21 cm测绘的数字管线

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摘要

3D mapping of matter distribution in the Universe through the 21 cm radio emission of atomic hydrogen (H I) is a complementary approach to optical surveys for the study of the Large Scale Structures, in particular for measuring the BAO (Baryon Acoustic Oscillation) scale up to redshifts z≤3, and therefore constraining dark energy parameters. We propose a novel method to map the H_I mass distribution in three dimensions in radio, without detecting or identifying individual compact sources. This method would require an instrument with a large instantaneous bandwidth (≥100 MHz) and high sensitivity, while a rather modest angular resolution (~10 arcmin) should be sufficient. These requirements can be met by a dense interferometric array or a phased array (FPA) in the focal plane of a large primary reflector, representing a total collecting area of a few thousand square meters with few hundred simultaneous beams covering a 20 to 100 square degrees field of view. We describe the development and qualification of an electronic and data processing system for digital radio interferometry and beam forming suitable for such instruments with several hundred receiver elements.
机译:通过21 cm原子氢无线电发射(HI)在宇宙中进行物质分布的3D映射是光学测量的一种补充方法,用于研究大型结构,尤其是用于测量BAO(重子声振荡)直至红移z≤3,因此限制了暗能量参数。我们提出了一种新颖的方法,可以在无线电中在三个维度上映射H_I质量分布,而无需检测或识别单个紧凑源。这种方法将要求仪器具有较大的瞬时带宽(≥100MHz)和高灵敏度,而适度的角度分辨率(〜10 arcmin)应足够。这些需求可以通过大型主反射器焦平面中的密集干涉式阵列或相控阵(FPA)来满足,该阵列表示总收集区域为几千平方米,同时几百个同时光束覆盖20至100平方度视野。我们描述了适用于具有数百个接收器元件的此类仪器的数字无线电干涉测量和波束成形的电子和数据处理系统的开发和鉴定。

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