Distribution models of antennas in radio astronomy: Efficiency comparison of the golden spiral interferometry
Elio Quiroga Rodriguez

TL;DR
This paper compares various antenna configurations in radio astronomy interferometry, finding that the golden spiral offers superior UV coverage and image quality, making it the most effective design for high-resolution observations.
Contribution
It introduces a comprehensive comparison of antenna arrangements, highlighting the efficiency of the golden spiral configuration over traditional grid, random, and Y-shaped setups.
Findings
Golden spiral provides the most uniform UV coverage.
Grid configuration causes periodic gaps degrading image quality.
Y configuration achieves high resolution but lacks complete coverage.
Abstract
This work compares the performance of different antenna configurations in radio astronomy interferometry, including the golden spiral, a grid, a random arrangement, and the "Y" configuration similar to the Very Large Array. One hundred antennas are simulated in each configuration, and the resulting UV coverage and image quality are analyzed. The results show that the golden spiral provides more uniform UV coverage without significant gaps, which improves image quality by reducing sidelobes and artifacts. In comparison, the grid exhibits periodic structures in the UV coverage that can degrade image quality due to gaps and artifacts. The random arrangement offers more natural coverage but is less efficient in terms of resolution and sidelobe control. The "Y" configuration proves effective in achieving high resolution along its arms but lacks complete coverage in certain directions, which…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
