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Lake Deployment of Southern Wide-field Gamma-ray Observatory (SWGO) Detector Units

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conference contribution
posted on 2025-04-09, 13:55 authored by H Goksu, W Hofmann, 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, BS González, F Guarino, A Guillén, F Haist, PM Hansen, JP Harding, J Hinton, 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, L Nellen, 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, CD Rho
The Southern Wide-field Gamma-ray Observatory (SWGO) will be a next-generation high altitude gamma-ray survey observatory in the southern hemisphere consisting of an array of water cherenkov detectors. With its energy range, wide field of view, large duty cycle and location it will complement the other existing and planned gamma-ray observatories. In this contribution we describe the lake concept for SWGO, an alternative to a HAWC-like design with individual water tanks and a LHAASO-style design with artificial ponds. In the lake concept, bladders filled with clean water are deployed near the surface of a natural lake, where each bladder is a light-tight stand-alone unit containing one or more photosensors. We will give an overview of the advantages and challenges for this design concept and describe the first results obtained from prototyping.

History

Author affiliation

School of Physics

Source

37th International Cosmic Ray Conference (ICRC2021)

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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