TY - JOUR
T1 - The search for high altitude sites in South America for the SWGO detector
AU - SWGO Collaboration
AU - Doro, M.
AU - Marques Moraes, A.
AU - Santander, M.
AU - Giammarchi, M.
AU - Mandat, D.
AU - Mendes, L. M.
AU - Bellido, J.
AU - Dib, C. O.
AU - May, S.
AU - Reisenegger, A.
AU - Rovero, A. C.
AU - Sandoval, A.
AU - Schussler, F.
AU - Springer, R. W.
AU - Torres, I.
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 - Assis, P.
AU - Bakalová, A.
AU - Barres de Almeida, U.
AU - Batković, I.
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 - Conceição, R.
AU - Consolati, G.
AU - Cotzomi Paleta, J.
AU - Dasso, S.
AU - De Angelis, A.
AU - De Bom, C. R.
AU - de la Fuente, E.
AU - de Souza, V.
AU - Depaoli, D.
AU - Martínez-Castro, J.
N1 - Funding Information:
Acknowledgement We thank César Ocampo and Pablo Pistoia (Atacama Astronomical Park, Chile) for providing useful information. The SWGO Collaboration acknowledges the support from the agencies and organizations listed here: https://www.swgo.org/SWGOWiki/doku.php?id=acknowledgements.
Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)
PY - 2022/3/18
Y1 - 2022/3/18
N2 - The Southern Wide-field Gamma-ray Observatory (SWGO) is a project for a new generation of extensive air shower front detectors, based primarily on the water Cherenkov technique, to be located in the Southern Hemisphere, where no other instrument of that kind is currently operating in the TeV gamma-ray energy range. The reference configuration of SWGO foresees an array of about 6, 000 water Cherenkov tanks deployed over a circle of 320 m diameter, about 80, 000 m2 area. In order to reach a sensitivity at energies around and below 1 TeV competitive with current and future detectors, SWGO will be placed at altitude above 4, 400 m a.s.l. Preliminary site searches have found several candidate sites in Argentina, Bolivia, Chile and Peru. The major challenge will be the water provision, considering that at least 105 m3 of water will be required. This poster will present the challenges and status of the SWGO site search in South America.
AB - The Southern Wide-field Gamma-ray Observatory (SWGO) is a project for a new generation of extensive air shower front detectors, based primarily on the water Cherenkov technique, to be located in the Southern Hemisphere, where no other instrument of that kind is currently operating in the TeV gamma-ray energy range. The reference configuration of SWGO foresees an array of about 6, 000 water Cherenkov tanks deployed over a circle of 320 m diameter, about 80, 000 m2 area. In order to reach a sensitivity at energies around and below 1 TeV competitive with current and future detectors, SWGO will be placed at altitude above 4, 400 m a.s.l. Preliminary site searches have found several candidate sites in Argentina, Bolivia, Chile and Peru. The major challenge will be the water provision, considering that at least 105 m3 of water will be required. This poster will present the challenges and status of the SWGO site search in South America.
UR - http://www.scopus.com/inward/record.url?scp=85145019679&partnerID=8YFLogxK
M3 - Artículo de la conferencia
AN - SCOPUS:85145019679
SN - 1824-8039
VL - 395
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 689
T2 - 37th International Cosmic Ray Conference, ICRC 2021
Y2 - 12 July 2021 through 23 July 2021
ER -