VAMOS: A pathfinder for the HAWC gamma-ray observatory
VAMOS1VAMOS is an acronym for: Verification and Assessment Measuring of Observatory Subsystem.1 was a prototype detector built in 2011 at an altitude of 4100m a.s.l. in the state of Puebla, Mexico. The aim of VAMOS was to finalize the design, construction techniques and data acquisition system of th...
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| Veröffentlicht in: | Astroparticle physics 2015-03, Vol.62 (C), p.125-133 |
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| creator | Abeysekara, A.U. Alfaro, R. Álvarez, J.D. Ángeles, F. Arceo, R. Arteaga-Velázquez, J.C. Avila-Aroche, A. Ayala Solares, H.A. Baughman, B.M. Bautista-Elivar, N. Belmont, E. Benítez, E. BenZvi, S.Y. Berley, D. Bernal, A. Bonilla Rosales, M. Braun, J. Caballero-Mora, K.S. Cabrera, I. Castañeda-Martínez, L. Castillo, M. Cotti, U. Cotzomi, J. de la Fuente, E. De León, C. DeYoung, T. Diaz-Azuara, A. Diaz-Cruz, L. DuVernois, M.A. Ellsworth, R.W. Fernandez, A. Fiorino, D.W. Fraija, N. Galindo, A. Garfias, F. González, A. González, L.X. Goodman, J.A. Grabski, V. Guzmán-Cerón, C. Hampel-Arias, Z. Hernández-Cervantes, L. Hüntemeyer, P. Imran, A. Karn, P. Kieda, D. Kunde, G.J. Lara, A. Lee, W.H. Lennarz, D. León Vargas, H. Linnemann, J.T. Longo, M. Luna-Garcia, R. Marinelli, A. Martínez, H. Martínez-Castro, J. McEnery, J. Mendoza Torres, E. Miranda-Romagnoli, P. Moreno, E. Mostafá, M. Nava, J. Nellen, L. Noriega-Papaqui, R. Oceguera-Becerra, T. Page, D.P. Patricelli, B. Pelayo, R. Pérez-Pérez, E.G. Pretz, J. Ramírez, I. Rentería, A. Rosa-González, D. Ruiz-Sala, F. Ruiz-Velasco, E.L. Ryan, J. Sacahui, J.R. Salazar, H. Sandoval, A. Schneider, M. Silich, S. Sinnis, G. Smith, A.J. Springer, R.W. Tepe, A. Torres, I. Valdés Galicia, J.F. Vanegas, P. Vázquez, A. Villaseñor, L. Wall, W. Westerhoff, S. Wisher, I.G. Wood, J. Yodh, G.B. Younk, P.W. Zaborov, D. Zepeda, A. Zhou, H. |
| description | VAMOS1VAMOS is an acronym for: Verification and Assessment Measuring of Observatory Subsystem.1 was a prototype detector built in 2011 at an altitude of 4100m a.s.l. in the state of Puebla, Mexico. The aim of VAMOS was to finalize the design, construction techniques and data acquisition system of the HAWC observatory. HAWC is an air-shower array currently under construction at the same site of VAMOS with the purpose to study the TeV sky. The VAMOS setup included six water Cherenkov detectors and two different data acquisition systems. It was in operation between October 2011 and May 2012 with an average live time of 30%. Besides the scientific verification purposes, the eight months of data were used to obtain the results presented in this paper: the detector response to the Forbush decrease of March 2012, and the analysis of possible emission, at energies above 30GeV, for long gamma-ray bursts GRB111016B and GRB120328B. |
| doi_str_mv | 10.1016/j.astropartphys.2014.08.004 |
| format | Article |
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Besides the scientific verification purposes, the eight months of data were used to obtain the results presented in this paper: the detector response to the Forbush decrease of March 2012, and the analysis of possible emission, at energies above 30GeV, for long gamma-ray bursts GRB111016B and GRB120328B.</description><identifier>ISSN: 0927-6505</identifier><identifier>EISSN: 1873-2852</identifier><identifier>DOI: 10.1016/j.astropartphys.2014.08.004</identifier><language>eng</language><publisher>Netherlands: Elsevier B.V</publisher><subject>Detector prototype ; Scientific verification ; TeV cosmic rays</subject><ispartof>Astroparticle physics, 2015-03, Vol.62 (C), p.125-133</ispartof><rights>2014 Elsevier 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P.</creatorcontrib><creatorcontrib>Vázquez, A.</creatorcontrib><creatorcontrib>Villaseñor, L.</creatorcontrib><creatorcontrib>Wall, W.</creatorcontrib><creatorcontrib>Westerhoff, S.</creatorcontrib><creatorcontrib>Wisher, I.G.</creatorcontrib><creatorcontrib>Wood, J.</creatorcontrib><creatorcontrib>Yodh, G.B.</creatorcontrib><creatorcontrib>Younk, P.W.</creatorcontrib><creatorcontrib>Zaborov, D.</creatorcontrib><creatorcontrib>Zepeda, A.</creatorcontrib><creatorcontrib>Zhou, H.</creatorcontrib><title>VAMOS: A pathfinder for the HAWC gamma-ray observatory</title><title>Astroparticle physics</title><description>VAMOS1VAMOS is an acronym for: Verification and Assessment Measuring of Observatory Subsystem.1 was a prototype detector built in 2011 at an altitude of 4100m a.s.l. in the state of Puebla, Mexico. 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Besides the scientific verification purposes, the eight months of data were used to obtain the results presented in this paper: the detector response to the Forbush decrease of March 2012, and the analysis of possible emission, at energies above 30GeV, for long gamma-ray bursts GRB111016B and GRB120328B.</description><subject>Detector prototype</subject><subject>Scientific verification</subject><subject>TeV cosmic 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B.V</general><general>Elsevier</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>20150301</creationdate><title>VAMOS: A pathfinder for the HAWC gamma-ray observatory</title><author>Abeysekara, A.U. ; Alfaro, R. ; Álvarez, J.D. ; Ángeles, F. ; Arceo, R. ; Arteaga-Velázquez, J.C. ; Avila-Aroche, A. ; Ayala Solares, H.A. ; Baughman, B.M. ; Bautista-Elivar, N. ; Belmont, E. ; Benítez, E. ; BenZvi, S.Y. ; Berley, D. ; Bernal, A. ; Bonilla Rosales, M. ; Braun, J. ; Caballero-Mora, K.S. ; Cabrera, I. ; Castañeda-Martínez, L. ; Castillo, M. ; Cotti, U. ; Cotzomi, J. ; de la Fuente, E. ; De León, C. ; DeYoung, T. ; Diaz-Azuara, A. ; Diaz-Cruz, L. ; DuVernois, M.A. ; Ellsworth, R.W. ; Fernandez, A. ; Fiorino, D.W. ; Fraija, N. ; Galindo, A. ; Garfias, F. ; González, A. ; González, L.X. ; Goodman, J.A. ; Grabski, V. ; Guzmán-Cerón, C. ; Hampel-Arias, Z. ; Hernández-Cervantes, L. ; Hüntemeyer, P. ; Imran, A. ; Karn, P. ; Kieda, D. ; Kunde, G.J. ; Lara, A. ; Lee, W.H. ; Lennarz, D. ; León Vargas, H. ; Linnemann, J.T. ; Longo, M. ; Luna-Garcia, R. ; Marinelli, A. ; Martínez, H. ; Martínez-Castro, J. ; McEnery, J. ; Mendoza Torres, E. ; Miranda-Romagnoli, P. ; Moreno, E. ; Mostafá, M. ; Nava, J. ; Nellen, L. ; Noriega-Papaqui, R. ; Oceguera-Becerra, T. ; Page, D.P. ; Patricelli, B. ; Pelayo, R. ; Pérez-Pérez, E.G. ; Pretz, J. ; Ramírez, I. ; Rentería, A. ; Rosa-González, D. ; Ruiz-Sala, F. ; Ruiz-Velasco, E.L. ; Ryan, J. ; Sacahui, J.R. ; Salazar, H. ; Sandoval, A. ; Schneider, M. ; Silich, S. ; Sinnis, G. ; Smith, A.J. ; Springer, R.W. ; Tepe, A. ; Torres, I. ; Valdés Galicia, J.F. ; Vanegas, P. ; Vázquez, A. ; Villaseñor, L. ; Wall, W. ; Westerhoff, S. ; Wisher, I.G. ; Wood, J. ; Yodh, G.B. ; Younk, P.W. ; Zaborov, D. ; Zepeda, A. ; Zhou, H.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c473t-2b503e2ffca7c130587540e527c8077969afce2172f9344a3894db172f924fbe3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Detector prototype</topic><topic>Scientific verification</topic><topic>TeV cosmic rays</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Abeysekara, A.U.</creatorcontrib><creatorcontrib>Alfaro, R.</creatorcontrib><creatorcontrib>Álvarez, J.D.</creatorcontrib><creatorcontrib>Ángeles, F.</creatorcontrib><creatorcontrib>Arceo, R.</creatorcontrib><creatorcontrib>Arteaga-Velázquez, J.C.</creatorcontrib><creatorcontrib>Avila-Aroche, A.</creatorcontrib><creatorcontrib>Ayala Solares, H.A.</creatorcontrib><creatorcontrib>Baughman, B.M.</creatorcontrib><creatorcontrib>Bautista-Elivar, N.</creatorcontrib><creatorcontrib>Belmont, 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R.</creatorcontrib><creatorcontrib>Marinelli, A.</creatorcontrib><creatorcontrib>Martínez, H.</creatorcontrib><creatorcontrib>Martínez-Castro, J.</creatorcontrib><creatorcontrib>McEnery, J.</creatorcontrib><creatorcontrib>Mendoza Torres, E.</creatorcontrib><creatorcontrib>Miranda-Romagnoli, P.</creatorcontrib><creatorcontrib>Moreno, E.</creatorcontrib><creatorcontrib>Mostafá, M.</creatorcontrib><creatorcontrib>Nava, J.</creatorcontrib><creatorcontrib>Nellen, L.</creatorcontrib><creatorcontrib>Noriega-Papaqui, R.</creatorcontrib><creatorcontrib>Oceguera-Becerra, T.</creatorcontrib><creatorcontrib>Page, D.P.</creatorcontrib><creatorcontrib>Patricelli, B.</creatorcontrib><creatorcontrib>Pelayo, R.</creatorcontrib><creatorcontrib>Pérez-Pérez, E.G.</creatorcontrib><creatorcontrib>Pretz, J.</creatorcontrib><creatorcontrib>Ramírez, I.</creatorcontrib><creatorcontrib>Rentería, A.</creatorcontrib><creatorcontrib>Rosa-González, D.</creatorcontrib><creatorcontrib>Ruiz-Sala, 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P.W.</creatorcontrib><creatorcontrib>Zaborov, D.</creatorcontrib><creatorcontrib>Zepeda, A.</creatorcontrib><creatorcontrib>Zhou, H.</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Astroparticle physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Abeysekara, A.U.</au><au>Alfaro, R.</au><au>Álvarez, J.D.</au><au>Ángeles, F.</au><au>Arceo, R.</au><au>Arteaga-Velázquez, J.C.</au><au>Avila-Aroche, A.</au><au>Ayala Solares, H.A.</au><au>Baughman, B.M.</au><au>Bautista-Elivar, N.</au><au>Belmont, E.</au><au>Benítez, E.</au><au>BenZvi, S.Y.</au><au>Berley, D.</au><au>Bernal, A.</au><au>Bonilla Rosales, M.</au><au>Braun, J.</au><au>Caballero-Mora, K.S.</au><au>Cabrera, I.</au><au>Castañeda-Martínez, L.</au><au>Castillo, M.</au><au>Cotti, U.</au><au>Cotzomi, J.</au><au>de la Fuente, E.</au><au>De León, C.</au><au>DeYoung, T.</au><au>Diaz-Azuara, A.</au><au>Diaz-Cruz, L.</au><au>DuVernois, M.A.</au><au>Ellsworth, R.W.</au><au>Fernandez, A.</au><au>Fiorino, D.W.</au><au>Fraija, N.</au><au>Galindo, A.</au><au>Garfias, F.</au><au>González, A.</au><au>González, L.X.</au><au>Goodman, J.A.</au><au>Grabski, V.</au><au>Guzmán-Cerón, C.</au><au>Hampel-Arias, Z.</au><au>Hernández-Cervantes, L.</au><au>Hüntemeyer, P.</au><au>Imran, A.</au><au>Karn, P.</au><au>Kieda, D.</au><au>Kunde, G.J.</au><au>Lara, A.</au><au>Lee, W.H.</au><au>Lennarz, D.</au><au>León Vargas, H.</au><au>Linnemann, J.T.</au><au>Longo, M.</au><au>Luna-Garcia, R.</au><au>Marinelli, A.</au><au>Martínez, H.</au><au>Martínez-Castro, J.</au><au>McEnery, J.</au><au>Mendoza Torres, E.</au><au>Miranda-Romagnoli, P.</au><au>Moreno, E.</au><au>Mostafá, M.</au><au>Nava, J.</au><au>Nellen, L.</au><au>Noriega-Papaqui, R.</au><au>Oceguera-Becerra, T.</au><au>Page, D.P.</au><au>Patricelli, B.</au><au>Pelayo, R.</au><au>Pérez-Pérez, E.G.</au><au>Pretz, J.</au><au>Ramírez, I.</au><au>Rentería, A.</au><au>Rosa-González, D.</au><au>Ruiz-Sala, F.</au><au>Ruiz-Velasco, E.L.</au><au>Ryan, J.</au><au>Sacahui, J.R.</au><au>Salazar, H.</au><au>Sandoval, A.</au><au>Schneider, M.</au><au>Silich, S.</au><au>Sinnis, G.</au><au>Smith, A.J.</au><au>Springer, R.W.</au><au>Tepe, A.</au><au>Torres, I.</au><au>Valdés Galicia, J.F.</au><au>Vanegas, P.</au><au>Vázquez, A.</au><au>Villaseñor, L.</au><au>Wall, W.</au><au>Westerhoff, S.</au><au>Wisher, I.G.</au><au>Wood, J.</au><au>Yodh, G.B.</au><au>Younk, P.W.</au><au>Zaborov, D.</au><au>Zepeda, A.</au><au>Zhou, H.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>VAMOS: A pathfinder for the HAWC gamma-ray observatory</atitle><jtitle>Astroparticle physics</jtitle><date>2015-03-01</date><risdate>2015</risdate><volume>62</volume><issue>C</issue><spage>125</spage><epage>133</epage><pages>125-133</pages><issn>0927-6505</issn><eissn>1873-2852</eissn><abstract>VAMOS1VAMOS is an acronym for: Verification and Assessment Measuring of Observatory Subsystem.1 was a prototype detector built in 2011 at an altitude of 4100m a.s.l. in the state of Puebla, Mexico. The aim of VAMOS was to finalize the design, construction techniques and data acquisition system of the HAWC observatory. HAWC is an air-shower array currently under construction at the same site of VAMOS with the purpose to study the TeV sky. The VAMOS setup included six water Cherenkov detectors and two different data acquisition systems. It was in operation between October 2011 and May 2012 with an average live time of 30%. Besides the scientific verification purposes, the eight months of data were used to obtain the results presented in this paper: the detector response to the Forbush decrease of March 2012, and the analysis of possible emission, at energies above 30GeV, for long gamma-ray bursts GRB111016B and GRB120328B.</abstract><cop>Netherlands</cop><pub>Elsevier B.V</pub><doi>10.1016/j.astropartphys.2014.08.004</doi><tpages>9</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0927-6505 |
| ispartof | Astroparticle physics, 2015-03, Vol.62 (C), p.125-133 |
| issn | 0927-6505 1873-2852 |
| language | eng |
| recordid | cdi_osti_scitechconnect_1250261 |
| source | Elsevier ScienceDirect Journals |
| subjects | Detector prototype Scientific verification TeV cosmic rays |
| title | VAMOS: A pathfinder for the HAWC gamma-ray observatory |
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