Development of the LAGO Project in Chiapas-Mexico
The Latin American Giant Observatory (LAGO) is an extended astroparticle observatory with the goal of studying Gamma Ray Bursts (among other extreme universe phenomena), space weather and atmospheric radiation at ground level. It consists of a network of several Water Cherenkov Detectors (WCD) locat...
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ftdatacite:10.48550/arxiv.1710.05224 2023-05-15T13:54:44+02:00 Development of the LAGO Project in Chiapas-Mexico Mora, Karen Salomé Caballero Hidalgo, Hugo de León Barbosa, Eduardo Moreno Ochoa, César Álvarez Reyes, Roberto Arceo Zahuantitla, Filiberto Hueyotl Kaufmann, Sarah Sánchez1, Luis Rodolfo Pérez Rodríguez, Elí Santos Tibolla, Omar Domínguez, Arnulfo Zepeda 2017 https://dx.doi.org/10.48550/arxiv.1710.05224 https://arxiv.org/abs/1710.05224 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Instrumentation and Detectors physics.ins-det Instrumentation and Methods for Astrophysics astro-ph.IM High Energy Physics - Experiment hep-ex FOS Physical sciences Preprint Article article CreativeWork 2017 ftdatacite https://doi.org/10.48550/arxiv.1710.05224 2022-04-01T10:16:43Z The Latin American Giant Observatory (LAGO) is an extended astroparticle observatory with the goal of studying Gamma Ray Bursts (among other extreme universe phenomena), space weather and atmospheric radiation at ground level. It consists of a network of several Water Cherenkov Detectors (WCD) located at different sites and different latitudes along the American Continent (from Mexico up to the Antarctic region). Another interest of LAGO is to encourage and support the development of experimental basic research in Latin America, mainly with low cost equipment. In the case of Chiapas, Mexico, the experimental astroparticle physics activity was limited, up to now, to data analysis from other detectors located far away from the region. Thanks to the collaboration within LAGO, the deployment of one WCD is ongoing at the Universidad Autónoma de Chiapas (UNACH). This will allow, for the first time in the region, to train students and researchers in the deployment processes. Till now the setup of the signal-processing electronics has been performed and the characterization of the photomultiplier tube is currently being done. The main, short-term goal is to install one WCD on top of the Tacaná volcano in Chiapas in a short term. The status of the work is presented. : International Cosmic Ray Conference, Busan, Korea, 10-20 July, 2017 https://pos.sissa.it/301/ Report Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology) Antarctic The Antarctic |
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Instrumentation and Detectors physics.ins-det Instrumentation and Methods for Astrophysics astro-ph.IM High Energy Physics - Experiment hep-ex FOS Physical sciences |
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Instrumentation and Detectors physics.ins-det Instrumentation and Methods for Astrophysics astro-ph.IM High Energy Physics - Experiment hep-ex FOS Physical sciences Mora, Karen Salomé Caballero Hidalgo, Hugo de León Barbosa, Eduardo Moreno Ochoa, César Álvarez Reyes, Roberto Arceo Zahuantitla, Filiberto Hueyotl Kaufmann, Sarah Sánchez1, Luis Rodolfo Pérez Rodríguez, Elí Santos Tibolla, Omar Domínguez, Arnulfo Zepeda Development of the LAGO Project in Chiapas-Mexico |
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Instrumentation and Detectors physics.ins-det Instrumentation and Methods for Astrophysics astro-ph.IM High Energy Physics - Experiment hep-ex FOS Physical sciences |
description |
The Latin American Giant Observatory (LAGO) is an extended astroparticle observatory with the goal of studying Gamma Ray Bursts (among other extreme universe phenomena), space weather and atmospheric radiation at ground level. It consists of a network of several Water Cherenkov Detectors (WCD) located at different sites and different latitudes along the American Continent (from Mexico up to the Antarctic region). Another interest of LAGO is to encourage and support the development of experimental basic research in Latin America, mainly with low cost equipment. In the case of Chiapas, Mexico, the experimental astroparticle physics activity was limited, up to now, to data analysis from other detectors located far away from the region. Thanks to the collaboration within LAGO, the deployment of one WCD is ongoing at the Universidad Autónoma de Chiapas (UNACH). This will allow, for the first time in the region, to train students and researchers in the deployment processes. Till now the setup of the signal-processing electronics has been performed and the characterization of the photomultiplier tube is currently being done. The main, short-term goal is to install one WCD on top of the Tacaná volcano in Chiapas in a short term. The status of the work is presented. : International Cosmic Ray Conference, Busan, Korea, 10-20 July, 2017 https://pos.sissa.it/301/ |
format |
Report |
author |
Mora, Karen Salomé Caballero Hidalgo, Hugo de León Barbosa, Eduardo Moreno Ochoa, César Álvarez Reyes, Roberto Arceo Zahuantitla, Filiberto Hueyotl Kaufmann, Sarah Sánchez1, Luis Rodolfo Pérez Rodríguez, Elí Santos Tibolla, Omar Domínguez, Arnulfo Zepeda |
author_facet |
Mora, Karen Salomé Caballero Hidalgo, Hugo de León Barbosa, Eduardo Moreno Ochoa, César Álvarez Reyes, Roberto Arceo Zahuantitla, Filiberto Hueyotl Kaufmann, Sarah Sánchez1, Luis Rodolfo Pérez Rodríguez, Elí Santos Tibolla, Omar Domínguez, Arnulfo Zepeda |
author_sort |
Mora, Karen Salomé Caballero |
title |
Development of the LAGO Project in Chiapas-Mexico |
title_short |
Development of the LAGO Project in Chiapas-Mexico |
title_full |
Development of the LAGO Project in Chiapas-Mexico |
title_fullStr |
Development of the LAGO Project in Chiapas-Mexico |
title_full_unstemmed |
Development of the LAGO Project in Chiapas-Mexico |
title_sort |
development of the lago project in chiapas-mexico |
publisher |
arXiv |
publishDate |
2017 |
url |
https://dx.doi.org/10.48550/arxiv.1710.05224 https://arxiv.org/abs/1710.05224 |
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Antarctic The Antarctic |
geographic_facet |
Antarctic The Antarctic |
genre |
Antarc* Antarctic |
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Antarc* Antarctic |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1710.05224 |
_version_ |
1766260819166756864 |