WAsp is a new scale-sensitive deconvolution algorithm for wide-band radio interferometry that reduces wide-scale residuals and spectral index errors by integrating improved Asp-Clean into MS-MFS.
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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.IM 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
Describes a distributed, memory-aware implementation of the widefield measurement operator for radio interferometry that decomposes into w-bin operators and optionally uses holographic matrices.
A review of Faraday Rotation Measure Synthesis techniques and SKA Array Assembly stages for high-resolution Faraday tomography of cosmic magnetic structures.
citing papers explorer
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WAsp: The Wideband (W) Adaptive-Scale Pixel (Asp) Deconvolution Algorithm for Interferometric Imaging
WAsp is a new scale-sensitive deconvolution algorithm for wide-band radio interferometry that reduces wide-scale residuals and spectral index errors by integrating improved Asp-Clean into MS-MFS.
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A distributed resource-adaptive implementation of the widefield radio-interferometric measurement model for scalable image formation
Describes a distributed, memory-aware implementation of the widefield measurement operator for radio interferometry that decomposes into w-bin operators and optionally uses holographic matrices.
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Faraday Tomography with the SKA: A New Era of Cosmic Magnetism Studies
A review of Faraday Rotation Measure Synthesis techniques and SKA Array Assembly stages for high-resolution Faraday tomography of cosmic magnetic structures.