English

Toward the End-To-End Optimization of the SWGO Array Layout

Instrumentation and Methods for Astrophysics 2025-05-12 v3 High Energy Astrophysical Phenomena

Abstract

In this document we consider the problem of finding the optimal layout for the array of water Cherenkov detectors proposed by the SWGO collaboration to study very-high-energy gamma rays in the southern hemisphere. We develop a continuous model of the secondary particles produced by atmospheric showers initiated by high-energy gamma rays and protons, and build an optimization pipeline capable of identifying the most promising configuration of the detector elements. The pipeline employs stochastic gradient descent to maximize a utility function aligned with the scientific goals of the experiment. We demonstrate how the software is capable of finding the global maximum in the high-dimensional parameter space, and discuss its performance and limitations.

Keywords

Cite

@article{arxiv.2310.01857,
  title  = {Toward the End-To-End Optimization of the SWGO Array Layout},
  author = {Tommaso Dorigo and Max Aehle and Cornelia Arcaro and Muhammad Awais and Fabiola Bergamaschi and Julien Donini and Michele Doro and Nicolas R. Gauger and Rafael Izbicki and Jan Kieseler and Ann Lee and Luca Masserano and Federico Nardi and Raaghav Rajesh and Luis Recabarren Vergara and Alexander Shen},
  journal= {arXiv preprint arXiv:2310.01857},
  year   = {2025}
}

Comments

40 pages, 23 figures. Accepted for publication in Nuclear Physics B

R2 v1 2026-06-28T12:39:11.230Z