The Latin American Giant Observatory (LAGO) capabilities for detecting gamma ray bursts
C. Sarmiento-Cano, H. Asorey, J. R. Sacahui, L. Otiniano, I. Sidelnik, V. Agosín, A. Alberto, C. Alvarez, J. Araya, R. Arceo, O. Areso, L. H. Arnaldi, M. Audelo, M. G. Ballina-Escobar, D. C. Becerra-Villamizar, X. Bertou, K. S. Caballero-Mora, R. Caiza, R. Calderón-Ardila, J. Calle, A. C. Fauth, E....
C. Sarmiento-Cano, H. Asorey, J. R. Sacahui, L. Otiniano, I. Sidelnik, V. Agosín, A. Alberto, C. Alvarez, J. Araya, R. Arceo, O. Areso, L. H. Arnaldi, M. Audelo, M. G. Ballina-Escobar, D. C. Becerra-Villamizar, X. Bertou, K. S. Caballero-Mora, R. Caiza, R. Calderón-Ardila, J. Calle, A. C. Fauth, E. C. Jarrin, L. E. C. Delacroix, C. Castromonte, D. Cazar-Ramírez, D. Cogollo, D. A. C. Borja, R. Conde, J. Cotzomi, D. Dallara, S. Dasso, R. Aguiar, A. Albuquerque, J. H. A. P. Reis, H. De León, R. deLeón-Barrios, D. Domínguez, M. Echiburu, M. González, M. G. Berisso, J. G. Casadiegos, A. M. Gulisano, J. C. Helo, C. A. H. Condori, J. E. Ise, G. K. M. Nascimento, M. A. L. de Oliveira, F. L. Miletto, V. P. Luzio, F. Machado, J. F. Mancilla-Caceres, D. Manriquez, A. Martínez-Méndez, O. Martinez, R. Mayo-García, L. G. Mijangos, P. Miranda, M. G. Molina, I. R. Morales, O. G. Morales-Olivares, E. Moreno-Barbosa, P. Muñoz, C. Nina, L. A. Núñez, L. Otininano, R. Pagán-Muñoz, K. M. Parada-Jaime, H. M. Parada-Villamizar, R. Parra, J. Peña-Rodríguez, M. Pereira, Y. A. Perez-Cuevas, H. Perez, J. Pisco-Guabave, M. Raljevic, M. Ramelli, C. Ramírez, H. Rivera, L. T. Rubinstein, A. J. Rubio-Montero, H. Salazar, N. Salomón, J. Samanes, N. A. Santos, M. B. Silva, O. Soto, M. Suárez-Durán, M. Subieta Vasquez, C. Terrazas, R. Ticona, T. T. Peralta, P. A. Ulloa, Z. R. Urrutia, N. Vásquez, A. Vázquez-Ramírez, A. Vega, P. Vega, J. Vega, A. Vesga-Ramirez, D. Vitoreti, R. W. Sobrinho and LAGO Collaboration
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Este artigo foi apresentado no evento International Cosmic Ray Conference, 2021
Agradecimentos: CSC, IS and HA acknowledge the support of CONICET and CNEA. This work was partly carried out within the ’European Open Science Cloud - Expanding Capacities by building Capabilities’ (EOSC-SYNERGY) project, founded by the European Commission’ Horizon 2020 RI Programme under Grant...
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Agradecimentos: CSC, IS and HA acknowledge the support of CONICET and CNEA. This work was partly carried out within the ’European Open Science Cloud - Expanding Capacities by building Capabilities’ (EOSC-SYNERGY) project, founded by the European Commission’ Horizon 2020 RI Programme under Grant Agreement nº 857647. This work has been also partially carried out on the ITeDA cluster, we thank A.P.J. Sedoski Croce for his continuous support. The LAGO Collaboration is very thankful to all the participating institutions and to the Pierre Auger Collaboration for their continuous support
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Abstract: The Latin American Giant Observatory (LAGO) consists of a network of small water Cherenkov detectors (WCD) located at different sites in Latin America. It is a large aperture observatory sensitive to high energy gamma rays and due to its high duty cycle, LAGO constitutes a facility to...
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Abstract: The Latin American Giant Observatory (LAGO) consists of a network of small water Cherenkov detectors (WCD) located at different sites in Latin America. It is a large aperture observatory sensitive to high energy gamma rays and due to its high duty cycle, LAGO constitutes a facility to detect transient events from the ground. Gamma Ray Bursts (GRBs) are of the brightest transients detected, with typical energies in their prompt phase ranging from keV to MeV, but theoretical models predict emissions at higher energies in the early times of the afterglow emission, and recently GRB190114C was the first GRB detected at TeV energies by the MAGIC experiment. In this work, we present the results of the expected sensitivity of LAGO for possible events like GRB190114C. We performed simulations in four of the high altitude LAGO sites projected to assess the sensitivity of the Observatory for this kind of events, using the ARTI toolkit developed by LAGO. We simulate photon showers with different spectral slopes and energies from 200 GeV to 1 TeV using the parameters presented by MAGIC for the recorded event. We also present maps of field of view of the studied sites with the observed GRBs by Fermi-GBM from 2019 to 2021
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DOI: https://doi.org/10.22323/1.395.0929
Texto completo: https://pos.sissa.it/395/929
The Latin American Giant Observatory (LAGO) capabilities for detecting gamma ray bursts
C. Sarmiento-Cano, H. Asorey, J. R. Sacahui, L. Otiniano, I. Sidelnik, V. Agosín, A. Alberto, C. Alvarez, J. Araya, R. Arceo, O. Areso, L. H. Arnaldi, M. Audelo, M. G. Ballina-Escobar, D. C. Becerra-Villamizar, X. Bertou, K. S. Caballero-Mora, R. Caiza, R. Calderón-Ardila, J. Calle, A. C. Fauth, E....
C. Sarmiento-Cano, H. Asorey, J. R. Sacahui, L. Otiniano, I. Sidelnik, V. Agosín, A. Alberto, C. Alvarez, J. Araya, R. Arceo, O. Areso, L. H. Arnaldi, M. Audelo, M. G. Ballina-Escobar, D. C. Becerra-Villamizar, X. Bertou, K. S. Caballero-Mora, R. Caiza, R. Calderón-Ardila, J. Calle, A. C. Fauth, E. C. Jarrin, L. E. C. Delacroix, C. Castromonte, D. Cazar-Ramírez, D. Cogollo, D. A. C. Borja, R. Conde, J. Cotzomi, D. Dallara, S. Dasso, R. Aguiar, A. Albuquerque, J. H. A. P. Reis, H. De León, R. deLeón-Barrios, D. Domínguez, M. Echiburu, M. González, M. G. Berisso, J. G. Casadiegos, A. M. Gulisano, J. C. Helo, C. A. H. Condori, J. E. Ise, G. K. M. Nascimento, M. A. L. de Oliveira, F. L. Miletto, V. P. Luzio, F. Machado, J. F. Mancilla-Caceres, D. Manriquez, A. Martínez-Méndez, O. Martinez, R. Mayo-García, L. G. Mijangos, P. Miranda, M. G. Molina, I. R. Morales, O. G. Morales-Olivares, E. Moreno-Barbosa, P. Muñoz, C. Nina, L. A. Núñez, L. Otininano, R. Pagán-Muñoz, K. M. Parada-Jaime, H. M. Parada-Villamizar, R. Parra, J. Peña-Rodríguez, M. Pereira, Y. A. Perez-Cuevas, H. Perez, J. Pisco-Guabave, M. Raljevic, M. Ramelli, C. Ramírez, H. Rivera, L. T. Rubinstein, A. J. Rubio-Montero, H. Salazar, N. Salomón, J. Samanes, N. A. Santos, M. B. Silva, O. Soto, M. Suárez-Durán, M. Subieta Vasquez, C. Terrazas, R. Ticona, T. T. Peralta, P. A. Ulloa, Z. R. Urrutia, N. Vásquez, A. Vázquez-Ramírez, A. Vega, P. Vega, J. Vega, A. Vesga-Ramirez, D. Vitoreti, R. W. Sobrinho and LAGO Collaboration
The Latin American Giant Observatory (LAGO) capabilities for detecting gamma ray bursts
C. Sarmiento-Cano, H. Asorey, J. R. Sacahui, L. Otiniano, I. Sidelnik, V. Agosín, A. Alberto, C. Alvarez, J. Araya, R. Arceo, O. Areso, L. H. Arnaldi, M. Audelo, M. G. Ballina-Escobar, D. C. Becerra-Villamizar, X. Bertou, K. S. Caballero-Mora, R. Caiza, R. Calderón-Ardila, J. Calle, A. C. Fauth, E....
C. Sarmiento-Cano, H. Asorey, J. R. Sacahui, L. Otiniano, I. Sidelnik, V. Agosín, A. Alberto, C. Alvarez, J. Araya, R. Arceo, O. Areso, L. H. Arnaldi, M. Audelo, M. G. Ballina-Escobar, D. C. Becerra-Villamizar, X. Bertou, K. S. Caballero-Mora, R. Caiza, R. Calderón-Ardila, J. Calle, A. C. Fauth, E. C. Jarrin, L. E. C. Delacroix, C. Castromonte, D. Cazar-Ramírez, D. Cogollo, D. A. C. Borja, R. Conde, J. Cotzomi, D. Dallara, S. Dasso, R. Aguiar, A. Albuquerque, J. H. A. P. Reis, H. De León, R. deLeón-Barrios, D. Domínguez, M. Echiburu, M. González, M. G. Berisso, J. G. Casadiegos, A. M. Gulisano, J. C. Helo, C. A. H. Condori, J. E. Ise, G. K. M. Nascimento, M. A. L. de Oliveira, F. L. Miletto, V. P. Luzio, F. Machado, J. F. Mancilla-Caceres, D. Manriquez, A. Martínez-Méndez, O. Martinez, R. Mayo-García, L. G. Mijangos, P. Miranda, M. G. Molina, I. R. Morales, O. G. Morales-Olivares, E. Moreno-Barbosa, P. Muñoz, C. Nina, L. A. Núñez, L. Otininano, R. Pagán-Muñoz, K. M. Parada-Jaime, H. M. Parada-Villamizar, R. Parra, J. Peña-Rodríguez, M. Pereira, Y. A. Perez-Cuevas, H. Perez, J. Pisco-Guabave, M. Raljevic, M. Ramelli, C. Ramírez, H. Rivera, L. T. Rubinstein, A. J. Rubio-Montero, H. Salazar, N. Salomón, J. Samanes, N. A. Santos, M. B. Silva, O. Soto, M. Suárez-Durán, M. Subieta Vasquez, C. Terrazas, R. Ticona, T. T. Peralta, P. A. Ulloa, Z. R. Urrutia, N. Vásquez, A. Vázquez-Ramírez, A. Vega, P. Vega, J. Vega, A. Vesga-Ramirez, D. Vitoreti, R. W. Sobrinho and LAGO Collaboration
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