Conceição R, Assis P, Assunção F, Bakalová A, Barres de Almeida U, Bom CR, Correia J, De Angelis A, Dias L, González BS, Guillén A, La Mura G, Lourenço N, Machado P, Marques S, Mendes L, Pimenta M, Shellard R, Tomé B, Vicha J, Abreu P, Albert A, Angüner EO, Arcaro C, Arnaldi LH, Arteaga-Velázquez JC, 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, Consolati G, Cotzomi Paleta J, Dasso S, 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, Guarino F, 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, 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, Portes de Albuquerque M, 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, Torres Aguilar I, van Eldik C, Vergara-Quispe ID, Viana A, 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 next-generation gamma-ray observatory, currently in an R&D phase. The experiment is expected to have a large array of water Cherenkov detectors (WCD) placed at a high elevation (> 4.4 km a.s.l.) in South America. Here we present a WCD concept with reduced surface area and height of stations comprising four PMTs at the bottom. We show that it is possible to reach an excellent gamma/hadron discrimination by analysing the data gathered by this station with machine learning techniques. Such performance can be achieved by analysing the shower patterns at the ground or through the PMTs signal time structure to tag muons. Moreover, it is shown that the station's performance does not depend on the array configuration (dense or sparse) nor on the shower inclination (θ< 40◦). Such a concept reduces the cost associated with the transport of massive amounts of water to high elevation sites while keeping a high physics performance. Therefore, it could be a good candidate station for SWGO, enabling to reach good sensitivities from low energies (∼ 100 GeV) up to the PeV region, covering large ground surface areas (few square km).
APA:
Conceição, R., Assis, P., Assunção, F., Bakalová, A., Barres de Almeida, U., Bom, C.R.,... Zamalloa Jara, M.A. (2022). Gamma/hadron discrimination using a small-WCD with four PMTs. In Proceedings of Science. Virtual, Berlin, DE: Sissa Medialab Srl.
MLA:
Conceição, R., et al. "Gamma/hadron discrimination using a small-WCD with four PMTs." Proceedings of the 37th International Cosmic Ray Conference, ICRC 2021, Virtual, Berlin Sissa Medialab Srl, 2022.
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