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The search for high altitude sites in South America for the SWGO detector

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conference contribution
posted on 2025-04-09, 13:31 authored by M Doro, A Marques Moraes, M Santander, M Giammarchi, D Mandat, LM Mendes, J Bellido, CO Dib, S May, A Reisenegger, AC Rovero, A Sandoval, F Schussler, RW Springer, I Torres, J Vicha, P Abreu, A Albert, EO Angüner, C Arcaro, LH Arnaldi, JC Arteaga-Velázquez, P Assis, A Bakalová, U Barres de Almeida, I Batković, 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, D Dorner, 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, AG Mariazzi, M Mariotti, J Martínez-Castro, H Martínez-Huerta, DG Melo, LF Mendes, T Mineeva, A Mitchell, S Mohan, OG Morales Olivares, E Moreno-Barbosa, L Nellen, V Novotny, L Olivera-Nieto, E Orlando
The Southern Wide-field Gamma-ray Observatory (SWGO) is a project for a new generation of extensive air shower front detectors, based primarily on the water Cherenkov technique, to be located in the Southern Hemisphere, where no other instrument of that kind is currently operating in the TeV gamma-ray energy range. The reference configuration of SWGO foresees an array of about 6, 000 water Cherenkov tanks deployed over a circle of 320 m diameter, about 80, 000 m2 area. In order to reach a sensitivity at energies around and below 1 TeV competitive with current and future detectors, SWGO will be placed at altitude above 4, 400 m a.s.l. Preliminary site searches have found several candidate sites in Argentina, Bolivia, Chile and Peru. The major challenge will be the water provision, considering that at least 105 m3 of water will be required. This poster will present the challenges and status of the SWGO site search in South America.

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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