posted on 2025-04-09, 13:50authored byH Schoorlemmer, R Conceição, AJ Smith, P Abreu, A Albert, EO Angüner, C Arcaro, LH Arnaldi, JC Arteaga-Velázquez, P Assis, A Bakalová, UB 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, KSC Mora, SM Campos, A Chiavassa, L Chytka, G Consolati, JC 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, STG 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, AM Moraes, J Martínez-Castro, H Martínez-Huerta, S May, DG Melo, LF Mendes, LM Mendes, T Mineeva, A Mitchell, S Mohan, OGM Olivares, E Moreno-Barbosa, L Nellen, V Novotny, L Olivera-Nieto, E Orlando, M Pech, A Pichel, M Pimenta, MP de Albuquerque, E Prandini, MSR Cuchills, A Reisenegger
The Southern Wide-view Gamma-ray Observatory (SWGO) will be a next-generation gamma-ray observatory using a large array of particle detectors at a high elevation site in South America. This project is currently in a three years R&D phase in which the design will be optimised for cost and performance. Therefore it is crucial to efficiently evaluate the impact of different design options on the scientific objectives of the observatory. In this contribution, we will introduce the strategy and the simulation framework in which this evaluation takes place.
History
Author affiliation
School of Physics
Source
37th International Cosmic Ray Conference (ICRC2021)