Accès ouvert déclaré
2023
conference-paper
Status of the SWGO air shower reconstruction using a template-based likelihood method
Franziska Leitl, P. Abreu, A. Albert, Ruben Jose Alfaro, Alexander Alfonso, César Álvarez, Qi An, E. O. Angüner, Cornelia Arcaro, R. Arceo, Sandro Arias, Horacio Arnaldi, P. Assis, H. A. Ayala Solares, Alena Bakalová, U. Barres de Almeida, Ivana Batković, J. Bazo, Jose A. Bellido, E. Belmont, S. BenZvi, Abel Bernal, Wenyi Bian, C. Bigongiari, E. Bottacini, P. Brogueira, T. Bulik, G. Busetto, K. S. Caballero‐Mora, P. Camarri, Silvina Campos, Wenyu Cao, Zhe Cao, Zhenfu Cao, T. Capistrán, M. Cardillo, E. Carquín, A. Carramiñana, C. Castromonte, J. F. Chang, Oscar Chaparro, Shangming Chen, Marco Chianese, A. Chiavassa, Ladislav Chytka, Roberta Colallillo, R. Conceição, Giovanni Consolati, Raúl R. Cordero, Pedro J. Costa, J. Cotzomi, S. Dasso, A. De Angelis, P. Desiati, F. Di Pierro, G. Di Sciascio, Claudio Dib, B. L. Dingus, Julia Isabel Djuvsland, C. Dobrigkeit, Luis Miguel Domingues Mendes, T. Dorigo, M. Doro, A. C. dos Reis, Michael Du Vernois, Mauricio Echiburu, D. Elsäesser, K. Engel, T. Ergin, Francisco Espinoza, Ke Fang, Fernando Farfán Carreras, A. Fazzi, C. Feng, M. Feroci, N. Fraija, S. Fraija, A. Franceschini, S. Funk, Sayri Garcia, J. A. García-González, F. Garfias, Gwenael Giacinti, Lucio Gibilisco, Jonas Glombitza, Hazal Goksu, G. Gong, B. S. González, Magda Gonzalez, J. A. Goodman, Minhao Gu, F. Guarino, Shivangi Gupta, Fabian Haist, Hayk Hakobyan, Guangchao Han, Patricia María Hansen, J. Patrick Harding, Juan Carlos Helo, Ian Herzog, Hugo d. Hidalgo, J. A. Hinton, Kun Hu, Dezhi Huang, Petra Huentemeyer, F. Hueyotl‐Zahuantitla, A. Iriarte, Jasmina Isaković, Antonio Isolia, Vikas Joshi, Jakub Jurýšek, S Kaci, Fabio La Monaca, G. La Mura, Rodrigo Guedes Lang, Roxana Laspiur, Luigi Lavitola, J. S. H. Lee, Luigi Lessio, Cong Li, Jian Li, Kai Li, Tianyang Li, B. Liberti, Sujie Lin, Dong Liu, Jia Liu, Ruoyu Liu, F. Longo, Yu Luo, Jing Lv, Elena Macerata, K. Malone, Dušan Mandát, M. Manganaro, Mario Mariani, Analisa Mariazzi, M. Mariotti, Teresa Marrodan, Jesús Arjona Martínez, H. Martínez-Huerta, S. Medina, Diego Melo, Filipe Mendes, Erick Meza, Davide Miceli, S. Miozzi, Alison Mitchell, Andrea Molinario, Oscar G. Morales-Olivares, E. Moreno, A. Morselli, Eros Mossini, M. Mostafá, Fabio Muleri, F. Nardi, Alessandro Negro, L. Nellen, Vladimír Novotný, Mabel Osorio, Luis Otiniano, M. Peresano, G. Piano, A. Pichel, Marine Pihet, M. Pimenta, E. Prandini, Jiajun Qin, Erick Quispe, S. Rainò, E. Rangel, Andreas Reisenegger, Helena X. Ren, Filip Rescic, Brian Reville, Chang Dong Rho, Mario Riquelme, Gonzalo Rodriguez Fernandez, Youn Roh, Gustavo E. Romero, B. Rossi, Adrián Rovero, E. Ruiz-Velasco, Germán Ariel Salazar, Jorge Samanes, Federico Sánchez, A. Sandoval, M. Santander, Rinaldo Santonico, Gizele Lian P. Santos, Ninetta Saviano, Michael Schneider, M. Schneider, Harm Schoorlemmer, José Erandi Serna-Franco, Victor Serrano, A. J. Smith, Y. Son, Orlando Javier Soto Sandoval, R. W. Springer, Luiz Augusto Stuani, H. Sun, Ruiyi Tang, Z. Tang, M. Tavani, T. Terzić, Kirsten Tollefson, B. Tomé, Ibrahim Daniel Torres, Ramiro Torres-Escobedo, Gian Carlo Trinchero, Rhiannon M. Turner, Laura Valore, C. van Eldik, Indira Vergara, A. Viana, J. Vícha, C. Vigorito, V. Vittorini, Bo Wang, J. S. Wang, Lingyu Wang, Xiaojie Wang, Xiangyu Wang, Xinsheng Wang, Z. Wang, Muhammad Mohsin Waqas, I. J. Watson, Felix Werner, R. White, C. H. Wiebusch, E. Willox, Frederik Wohlleben, Sha Wu, Shaoqiang Xi, Gang Xiao, Lili Yang, Ruizhi Yang, Raul Yanyachi, Z. G. Yao, Danilo Zavrtanik, Hong-Fei Zhang, Hai-Ming Zhang, Shaoru Zhang, Xiaopeng Zhang, Yuanping Zhang, Jing Zhao, Lei Zhao, Zhou Zhou, C. G. Zhu, Pengzhe Zhu, Xiong Zuo
1Citations signalées — pas une note de qualité
0Institutions déclarées
0Pays d’affiliation déclarés
Résumé fourni par la source
The Southern Wide-field Gamma-ray Observatory (SWGO) is a proposed facility for ground-based gamma-ray astronomy. It will consist of an array of water Cherenkov detectors to detect astrophysical gamma-rays mainly in the range of hundreds of GeV up to the PeV scale. To be constructed in South America, it will feature an approximately two-steradian field of view and a duty cycle close to 100%, which will complement the current generation of instruments by extending survey coverage to the Southern Hemisphere. As part of the development of the SWGO standard reconstruction framework, we employ a Monte Carlo template-based method to estimate the properties of the primary gamma-ray (such as core position and energy). In this method, an observed lateral amplitude distribution of a gamma-ray-induced air shower is fitted to the expected probability distribution stored in the templates. We validate this approach by estimating the energy performance for one of the currently investigated test array and detector unit configurations for SWGO.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Contrôle bibliographique ouvert
DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.
- Titre Crossref
- Status of the SWGO air shower reconstruction using a template-based likelihood method
- Date Crossref
- 17/08/2023
- Éditeur
- SISSA Medialab
- Type
- proceedings-article
Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude et ne compte pas comme une seconde source scientifique indépendante.
Sujets associés
Astrophysics and Cosmic PhenomenaGamma-ray bursts and supernovaeNeutrino Physics Research