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

Doro, M.; Marques Moraes, A.; Santander, M.; Giammarchi, M.; Mandat, D.; Mendes, L. M.; Bellido, J.; Dib, C. O.; May, S.; Reisenegger, A.; Rovero, A. C.; Sandoval, A.; Schussler, F.; Springer, R. W.; Torres, I.; Vicha, J.; Abreu, P.; Albert, A.; Anguner, E. O.; Arcaro, C.; Arnaldi, L. H.; Arteaga-Velazquez, J. C.; Assis, P.; Bakalova, A.; Barres de Almeida, U.; Batkovic, I.; Belmont-Moreno, E.; Bisconti, F.; Blanco, A.; Bohacova, M.; Bottacini, E.; Bretz, T.; Brisbois, C.; Brogueira, P.; Brown, A. M.; Bulik, T.; Caballero Mora, K. S.; Campos, S. M.; Chiavassa, A.; Chytka, L.; Conceicao, R.; Consolati, G.; Cotzomi Paleta, J.; Dasso, S.; De Angelis, A.; De Bom, C. R.; de la Fuente, E.; de Souza, V.; Depaoli, D.; Di Sciascio, G.; Dorner, D.; Du Vernois, M.; Ergin, T.; Fan, K. L.; Fraija, N.; Funk, S.; Garcia, J. I.; Garcia-Gonzalez, J. A.; Garcia Roca, S. T.; Giacinti, G.; Goksu, H.; Gonzalez, B. S.; Guarino, F.; Guillen, A.; Haist, F.; Hansen, P. M.; Harding, J. P.; Hinton, J.; Hofmann, W.; Hona, B.; Hoyos, D.; Huentemeyer, P.; Hueyotl-Zahuantitla, F.; Insolia, A.; Janecek, P.; Joshi, V.; Khelifi, B.; Kunwar, S.; La Mura, G.; Lapington, J.; Laspiur, M. R.; Leitl, F.; Longo, F.; Lopes, L.; Lopez-Coto, R.; Mariazzi, A. G.; Mariotti, M.; Martinez-Castro, J.; Martinez-Huerta, H.; Melo, D. G.; Mendes, L. F.; Mineeva, T.; Mitchell, A.; Mohan, S.; Morales Olivares, O. G.; Moreno-Barbosa, E.; Nellen, L.; Novotny, V.; Olivera-Nieto, L.; Orlando, E.; Pech, M.; Pichel, A.; Pimenta, M.; Portes de Albuquerque, M.; Prandini, E.; Rado Cuchills, M. S.; Reville, B.; Rho, C. D.; Ruiz-Velasco, E.; Salazar, G. A.; Schoorlemmer, H.; Schussler, F.; Serrano, V. H.; Shellard, R. C.; Sinha, A.; Smith, A. J.; Surajbali, P.; Tome, B.; Torres Aguilar, I.; van Eldik, C.; Vergara-Quispe, I. D.; Viana, A.; Vicha, J.; Vigorito, C. F.; Wang, X.; Werner, F.; White, R.; Zamalloa Jara, M. A.

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.