Abreu P, Albert A, Angüner EO, Arcaro C, Arnaldi LH, Arteaga-Velázquez JC, Assis P, Bakalová A, de Almeida UB, Batković I, Bellido J, Belmont-Moreno E, Bisconti F, Blanco A, Bohacova M, Bottacini E, Bretz T, Brisbois C, Brogueira P, Brown AM, Bulik T, Caballero Mora KS, Campos SM, Chiavassa A, Chytka L, Conceição R, Consolati G, Cotzomi Paleta J, Dasso S, de Angelis A, De Bom CR, de la Fuente E, de Souza V, Depaoli D, Di Sciascio G, Dib CO, Dorner D, Doro M, Du Vernois M, Ergin T, Fan KL, Fraija N, Funk S, García JI, García-González JA, García Roca ST, Giacinti G, Goksu H, González BS, Guarino F, Guillén A, Haist F, Hansen PM, Harding JP, 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 MR, Leitl F, Longo F, Lopes L, López-Coto R, Mandat D, Mariazzi AG, Mariotti M, Marques Moraes A, Martínez-Castro J, Martínez-Huerta H, May S, Melo DG, Mendes LF, Mendes LM, Mineeva T, Mitchell A, Mohan S, Morales Olivares OG, Moreno-Barbosa E, Nellen L, Novotny V, Olivera-Nieto L, Orlando E, Pech M, Pichel A, Pimenta M, de Albuquerque MP, Prandini E, Rado Cuchills MS, Reisenegger A, Reville B, Rho CD, Rovero AC, Ruiz-Velasco E, Salazar GA, Sandoval A, Santander M, Schoorlemmer H, Schüssler F, Serrano VH, Shellard RC, Sinha A, Smith AJ, Surajbali P, Tomé B, Torres Aguilar I, van Eldik C, Vergara-Quispe ID, Viana A, Vícha J, Vigorito CF, Wang X, Werner F, White R, Zamalloa Jara MA (2022)
Publication Type: Conference contribution
Publication year: 2022
Publisher: Sissa Medialab Srl
Book Volume: 395
Conference Proceedings Title: Proceedings of Science
Event location: Virtual, Berlin
The Southern Wide-field Gamma-ray Observatory (SWGO) is the project to build a new extensive air shower particle detector for the observation of very-high-energy gamma-rays in South America. SWGO is currently planned for installation in the Southern Hemisphere, which grants it a unique science potential among ground-based gamma-ray detectors. It will complement the capabilities of CTA, working as a wide-field instrument for the monitoring of transient and variable phenomena, and will expand the sky coverage of Northern Hemisphere facilities like HAWC and LHAASO, thus granting access to the entire Galactic Plane and the Galactic Center. SWGO aims to achieve excellent sensitivity over a very large target energy range from about 100 GeV to the PeV, and improve on the performance of current sampling array instruments in all observational parameters, including energy and angular resolution, background rejection, and single-muon detection capabilities. The directives for the final observatory design will be given by a number of key science goals which are being defined over the course of the Project’s R&D phase. In this contribution we will present the core science topics and target performance goals that serve as benchmarks to guide SWGO’s design configuration.
APA:
Abreu, P., Albert, A., Angüner, E.O., Arcaro, C., Arnaldi, L.H., Arteaga-Velázquez, J.C.,... Zamalloa Jara, M.A. (2022). Benchmarking the Science for the Southern Wide-Field Gamma-ray Observatory (SWGO). In Proceedings of Science. Virtual, Berlin, DE: Sissa Medialab Srl.
MLA:
Abreu, P., et al. "Benchmarking the Science for the Southern Wide-Field Gamma-ray Observatory (SWGO)." Proceedings of the 37th International Cosmic Ray Conference, ICRC 2021, Virtual, Berlin Sissa Medialab Srl, 2022.
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