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Technological options for the Southern Wide-field Gamma-ray Observatory (SWGO) and current design status

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conference contribution
posted on 2025-04-09, 13:33 authored by F Werner, L Nellen, P Abreu, A Albert, EO Angüner, C Arcaro, LH Arnaldi, JC Arteaga-Velázquez, P Assis, A Bakalová, U Barres de Almeida, I Batković, J Bellido, E Belmont-Moreno, F Bisconti, A Blanco, M Bohacova, E Bottacini, T Bretz, C Brisbois, P Brogueira, AM Brown, T Bulik, KS Caballero Mora, SM Campos, A Chiavassa, L Chytka, R Conceição, G Consolati, J Cotzomi Paleta, S Dasso, A De Angelis, CR De Bom, E de la Fuente, V de Souza, D Depaoli, G Di Sciascio, CO Dib, D Dorner, M Doro, M Du Vernois, T Ergin, KL Fan, N Fraija, S Funk, JI García, JA García-González, ST García Roca, G Giacinti, H Goksu, BS González, F Guarino, A Guillén, F Haist, PM Hansen, JP Harding, J Hinton, W Hofmann, B Hona, D Hoyos, P Huentemeyer, F Hueyotl-Zahuantitla, A Insolia, P Janecek, V Joshi, B Khelifi, S Kunwar, G La Mura, J Lapington, MR Laspiur, F Leitl, F Longo, L Lopes, R Lopez-Coto, D Mandat, AG Mariazzi, M Mariotti, A Marques Moraes, J Martínez-Castro, H Martínez-Huerta, S May, DG Melo, LF Mendes, LM Mendes, T Mineeva, A Mitchell, S Mohan, OG Morales Olivares, E Moreno-Barbosa, V Novotny, L Olivera-Nieto, E Orlando, M Pech, A Pichel, M Pimenta, M Portes de Albuquerque, E Prandini, MS Rado Cuchills, A Reisenegger, B Reville
The SWGO Collaboration is in the process of designing and prototyping a wide field of view, high duty cycle complement to CTA and the existing ground-based particle detectors of the Northern Hemisphere (HAWC and LHAASO). In this contribution, we will compare the various technological options for designing the detector and present an overarching system design accommodating them. We will introduce a feasible reference configuration that is used for the first large-scale simulations and cost estimates, and show ongoing prototyping work focused on reaching a maintenance-free and cost-effective detector.

History

Version

  • VoR (Version of Record)

Published in

Proceedings of Science

Volume

395

Publisher

Sissa Medialab srl Partita

eissn

1824-8039

Copyright date

2022

Available date

2025-04-09

Language

en

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