Memory-efficient w-projection with the fast Gauss transform
classification
🌌 astro-ph.IM
keywords
arrayfastgaussperformancetransformw-projectionactualalgorithms
pith:ZNNRLY36 Add to your LaTeX paper
What is a Pith Number?\usepackage{pith}
\pithnumber{ZNNRLY36}
Prints a linked pith:ZNNRLY36 badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more
read the original abstract
We describe a method performing w-projection using the fast Gauss transform of Strain (1991). We derive the theoretical performance, and simulate the actual performance for a range of w for a canonical array. While our implementation is dominated by overheads, we argue that this approach could for the basis of a higher-performing algorithms with particular application to the Square Kilometer Array.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.