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Simulating the performance of the Southern Wide-view Gamma-ray Observatory

Authors :
Schoorlemmer, H.
Conceição, R.
Smith, A. J.
Abreu, P.
Albert, A.
Angüner, E. O.
Arcaro, C.
Arnaldi, L. H.
Arteaga-Velázquez, J. C.
Assis, P.
Bakalová, A.
Almeida, U. B.
Batković, I.
Bellido, J.
Belmont-Moreno, E.
Bisconti, F.
Blanco, A.
Bohacova, M.
Bottacini, E.
Bretz, T.
Brisbois, C.
Brogueira, P.
Brown, A. M.
Bulik, T.
Mora, K. S. C.
Campos, S. M.
Chiavassa, A.
Chytka, L.
Consolati, G.
Paleta, J. C.
Dasso, S.
Angelis, A.
Bom, C. R.
La Fuente, E.
Souza, V.
Depaoli, D.
Di Sciascio, G.
Dib, C. O.
Dorner, D.
Doro, M.
Du Vernois, M.
Ergin, T.
Fan, K. L.
Fraija, N.
Funk, S.
García, J. I.
García-González, J. A.
Roca, S. T. G.
Giacinti, G.
Goksu, H.
González, B. S.
Guarino, F.
Guillén, A.
Haist, F.
Hansen, P. M.
Harding, J. P.
Hinton, J.
Hofmann, W.
Hona, B.
Hoyos, D.
Huentemeyer, P.
Hueyotl-Zahuantitla, F.
Insolia, A.
Janecek, P.
Joshi, V.
Khelifi, B.
Samridha Kunwar
La Mura, G.
Lapington, J.
Laspiur, M. R.
Leitl, F.
Longo, F.
Lopes, L.
Lopez-Coto, R.
Mandat, D.
Mariazzi, A. G.
Mariotti, M.
Moraes, A. M.
Martínez-Castro, J.
Martínez-Huerta, H.
May, S.
Melo, D. G.
Mendes, L. F.
Mendes, L. M.
Mineeva, T.
Mitchell, A.
Mohan, S.
Olivares, O. G. M.
Moreno-Barbosa, E.
Nellen, L.
Novotny, V.
Olivera-Nieto, L.
Orlando, E.
Pech, M.
Pichel, A.
Pimenta, M.
Albuquerque, M. P.
Prandini, E.
Cuchills, M. S. R.
Reisenegger, A.
Reville, B.
Rho, C. D.
Rovero, A. C.
Ruiz-Velasco, E.
Salazar, G. A.
Sandoval, A.
Santander, M.
Schüssler, F.
Serrano, V. H.
Shellard, R. C.
Sinha, A.
Surajbali, P.
Tomé, B.
Aguilar, I. T.
Eldik, C.
Vergara-Quispe, I. D.
Viana, A.
Vícha, J.
Vigorito, C. F.
Wang, X.
Werner, F.
White, R.
Jara, M. A. Z.
Source :
CIÊNCIAVITAE, Scopus-Elsevier, Proceedings of Science

Abstract

The Southern Wide-view Gamma-ray Observatory (SWGO) will be a next-generation gamma-ray observatory using a large array of particle detectors at a high elevation site in South America. This project is currently in a three years R & D phase in which the design will be optimised for cost and performance. Therefore it is crucial to efficiently evaluate the impact of different design options on the scientific objectives of the observatory. In this contribution, we will introduce the strategy and the simulation framework in which this evaluation takes place.

Subjects

Subjects :
SWGO - Abteilung Hinton
Observatory
Astrophysics::High Energy Astrophysical Phenomena
Detector
Large array
Astrophysics::Instrumentation and Methods for Astrophysics
Elevation
Gamma ray
Phase (waves)
Environmental science
Remote sensing

Details

Database :
OpenAIRE
Journal :
CIÊNCIAVITAE, Scopus-Elsevier, Proceedings of Science
Accession number :
edsair.doi.dedup.....6a2eecc88a1969f23943428100ffc1d0

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