Author

R. Conceição
P. Assis
F. Assunção
A. Bakalová
U. Barres de Almeida
C. R. Bom
J. Correia
A. De Angelis
L. Dias
B. S. González
A. Guillén
G. La Mura
N. Lourenço
P. Machado
S. Marques
L. Mendes
M. Pimenta
R. Shellard
B. Tome
J. Vicha
P. Abreu
A. Albert
E. O. Anguner
C. Arcaro
L. H. Arnaldi
J. C. Artega-Velazquez
P. Assis
A. Bakalova
U. Barres de Almeda
I. Batkovic
J. Bellido
E. Belmont-Moreno
F. Bisconti
A. Blanco
M. Bohacova
E. Bottacini
T. Bretz
C. Brisbois
P. Brogueira
A. M. Brown
T. Bulik
K. S. Caballero Mora
S. M. Campos
A. Chiavassa
L. Chytka
R. Conceicao
G. Consolati
J. Cotzomi Paleta
S. Dasso
A. De Angelis
C. R. Bom
E. de la Fuente
V. de Souza
D. Depaoli
G. Di Sciascio
C. O. Dib
D. Dorner
M. Doro
M. Du Vernois
T. Ergin
K. L. Fan
N. Fraija
S. Funk
J. I. Garcia
J. A. Garcia-Gonzalez
S. T. Garcia Roca
G. Giacinti
H. Goksu
B. S. Gonzalez
F. Guarino
A. Guillen
F. Haist
P. M. Hansen
J. P. 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
M. R. Laspiur
F. Leitl
F. Longo
L. Lopes
R. Lopez-Coto
D. Mandat
A. G. Mariazzi
M. Mariotti
A. Marques Moraes
J. Martinez-Castro
H. Martinez-Huerta
S. May
D. G. Melo
L. F. Mendes
L. M. Mendes
T. Mineeva
A. Mitchell
S. Mohan
O. G. Morales Olivares
E. Moreno-Barbosa
L. Nellen
V. Novotny
L. Olivera-Nieto
E. Orlando
M. Pech
A. Pichel
M. Pimenta
M. Portes de Albuquerque
E. Prandini
M. S. Rado Cuchills
A. Reisenegger
B. Riville
C. D. Rho
A. C. Rovero
E. Ruiz-Velasco
G. A. Salazar
A. Sandoval
M. Santander
H. Schoorlemmer
F. Schussler
V. H. Serrano
R. C. Shellard
A. Sinha
A. J. Smith
P. Surajbali
B. Tome
I. Torres Aguilar
C. van Eldik
I. D. Vargara-Quispe
A. Viana
J. Vicha
C. F. Vigorito
Xiaojie Wang, Missouri University of Science and TechnologyFollow
F. Werner
R. White
M. A. Zamalloa Jara

Abstract

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 analyzing the data gathered by this station with machine learning techniques. Such performance can be achieved by analyzing 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).

Department(s)

Physics

Publication Status

Open Access

Comments

Fundação para a Ciência e a Tecnologia, Grant DL57/2016/cP1330/cT0002

International Standard Serial Number (ISSN)

1824-8039

Document Type

Article - Conference proceedings

Document Version

Citation

File Type

text

Language(s)

English

Rights

© 2025 Sissa Medialab Srl, All rights reserved.

Publication Date

18 Mar 2022

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