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Time-Regularized Blind Deconvolution Approach for Radio Interferometry

机译:用于无线电干涉测量的时间正常化的盲折叠方法

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Radio-interferometric imaging aims to estimate a sky intensity image from degraded undersampled Fourier measurements. At the dynamic range of interest to modern radio telescopes, the image reconstruction quality will be limited by the unknown time-dependent calibration kernels. Hence the need of performing joint image reconstruction and calibration, and consequently of solving a non-convex blind deconvolution problem. Extending our recent work where the calibration kernels are assumed to be smooth in space, we further assume in this work that the calibration kernels are smooth in time. In addition, an average sparsity prior is used for the estimation of the image of interest. The resulting high dimensional non-convex non-smooth minimization problem is then solved by leveraging an alternating forward-backward algorithm which benefits from well-established convergence guarantees. Our results show that time-regularization is effective in enhancing imaging quality.
机译:无线电干涉测量成像旨在估计来自劣化的傅立叶测量的天空强度图像。在现代无线电望远镜的动态范围内,图像重建质量将受到未知时间依赖校准内核的限制。因此,需要进行关节图像重建和校准,并因此解决非凸盲卷积问题。延长我们最近的工作,其中假设校准内核在空间中平滑,我们进一步假设校准内核及时平滑。此外,平均稀疏性用于估计感兴趣的图像。然后通过利用交替的前后算法来解决所得到的高维度非凸出的最小化问题,该算法从建立的良好的收敛保证中受益。我们的结果表明,时间正则化在提高成像质量方面是有效的。

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