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A randomised primal-dual algorithm for distributed radio-interferometric imaging

机译:分布式无线电干涉成像的随机原始对偶算法

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Next generation radio telescopes, like the Square Kilometre Array, will acquire an unprecedented amount of data for radio astronomy. The development of fast, parallelisable or distributed algorithms for handling such large-scale data sets is of prime importance. Motivated by this, we investigate herein a convex optimisation algorithmic structure, based on primal-dual forward-backward iterations, for solving the radio interferometric imaging problem. It can encompass any convex prior of interest. It allows for the distributed processing of the measured data and introduces further flexibility by employing a probabilistic approach for the selection of the data blocks used at a given iteration. We study the reconstruction performance with respect to the data distribution and we propose the use of nonuniform probabilities for the randomised updates. Our simulations show the feasibility of the randomisation given a limited computing infrastructure as well as important computational advantages when compared to state-of-the-art algorithmic structures.
机译:像平方公里阵列这样的下一代射电望远镜将为射电天文学获取前所未有的数据量。开发用于处理此类大规模数据集的快速,可并行化或分布式算法至关重要。出于此目的,我们在此研究一种基于原始-对偶向前-向后迭代的凸优化算法结构,用于解决无线电干涉成像问题。它可以包含任何感兴趣的凸先验。它允许对测量数据进行分布式处理,并通过采用概率方法来选择给定迭代中使用的数据块,从而引入了更大的灵活性。我们研究了关于数据分布的重建性能,并建议将非均匀概率用于随机更新。与最先进的算法结构相比,我们的仿真显示了在有限的计算基础结构的情况下随机化的可行性以及重要的计算优势。

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