TY - JOUR
T1 - Gamma/hadron discrimination using a small-WCD with four PMTs
AU - the SWGO Collaboration
AU - Conceição, R.
AU - Assis, P.
AU - Assunção, F.
AU - Bakalová, A.
AU - Barres de Almeida, U.
AU - Bom, C. R.
AU - Correia, J.
AU - De Angelis, A.
AU - Dias, L.
AU - González, B. S.
AU - Guillén, A.
AU - La Mura, G.
AU - Lourenço, N.
AU - Machado, P.
AU - Marques, S.
AU - Mendes, L.
AU - Pimenta, M.
AU - Shellard, R.
AU - Tomé, B.
AU - Vicha, J.
AU - Abreu, P.
AU - Albert, A.
AU - Angüner, E. O.
AU - Arcaro, C.
AU - Arnaldi, L. H.
AU - Arteaga-Velázquez, J. C.
AU - Batković, I.
AU - Bellido, J.
AU - Belmont-Moreno, E.
AU - Bisconti, F.
AU - Blanco, A.
AU - Bohacova, M.
AU - Bottacini, E.
AU - Bretz, T.
AU - Brisbois, C.
AU - Brogueira, P.
AU - Brown, A. M.
AU - Bulik, T.
AU - Caballero Mora, K. S.
AU - Campos, S. M.
AU - Chiavassa, A.
AU - Chytka, L.
AU - Consolati, G.
AU - Cotzomi Paleta, J.
AU - Dasso, S.
AU - De Bom, C. R.
AU - de la Fuente, E.
AU - de Souza, V.
AU - Depaoli, D.
AU - Marques Moraes, A.
N1 - Publisher Copyright:
© 2022 Sissa Medialab Srl. All rights reserved.
PY - 2022/3/18
Y1 - 2022/3/18
N2 - 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).
AB - 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).
UR - http://www.scopus.com/inward/record.url?scp=85125119378&partnerID=8YFLogxK
M3 - Conference article
AN - SCOPUS:85125119378
SN - 1824-8039
VL - 395
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 707
T2 - 37th International Cosmic Ray Conference, ICRC 2021
Y2 - 12 July 2021 through 23 July 2021
ER -