VAMOS: A pathfinder for the HAWC gamma-ray observatory

A. U. Abeysekara; R. Alfaro; C. Alvarez; J. D. Álvarez; F. Ángeles; R. Arceo; J. C. Arteaga-Velázquez; A. Avila-Aroche; H. A. Ayala Solares; C. Badillo; A. S. Barber; B. M. Baughman; N. Bautista-Elivar; J. Becerra Gonzalez; E. Belmont; E. Benítez; S. Y. Benzvi; D. Berley; A. Bernal; M. Bonilla Rosales; J. Braun; R. A. Caballero-Lopez; K. S. Caballero-Mora; I. Cabrera; A. Carramiñana; L. Castañeda-Martínez; M. Castillo; U. Cotti; J. Cotzomi; E. De La Fuente; C. De León; T. Deyoung; A. Diaz-Azuara; L. Diaz-Cruz; R. Diaz Hernandez; J. C. Díaz-Vélez; B. L. Dingus; D. Dultzin; M. A. Duvernois; R. W. Ellsworth; A. Fernandez; D. W. Fiorino; N. Fraija; A. Galindo; G. García-Torales; F. Garfias; A. González; L. X. González; M. M. González; J. A. Goodman; V. Grabski; M. Gussert; C. Guzmán-Cerón; Z. Hampel-Arias; J. P. Harding; L. Hernández-Cervantes; C. M. Hui; P. Hüntemeyer; A. Imran; A. Iriarte; P. Karn; D. Kieda; G. J. Kunde; R. Langarica; A. Lara; G. Lara; R. J. Lauer; W. H. Lee; D. Lennarz; H. León Vargas; E. C. Linares; J. T. Linnemann; M. Longo; R. Luna-Garcia; A. Marinelli; L. A. Martínez; H. Martínez; O. Martínez; J. Martínez-Castro; M. Martos; J. A.J. Matthews; J. McEnery; E. Mendoza Torres; P. Miranda-Romagnoli; E. Moreno; M. Mostafá; J. Nava; L. Nellen; M. Newbold; R. Noriega-Papaqui; T. Oceguera-Becerra; D. P. Page; B. Patricelli; R. Pelayo; E. G. Pérez-Pérez; J. Pretz; I. Ramírez; A. Rentería; C. Rivière; D. Rosa-González; F. Ruiz-Sala; E. L. Ruiz-Velasco; J. Ryan; J. R. Sacahui; H. Salazar; F. Salesa; A. Sandoval; E. Santos; M. Schneider; S. Silich; G. Sinnis; A. J. Smith; K. Sparks Woodle; R. W. Springer; F. Suarez; I. Taboada; A. Tepe; P. A. Toale; K. Tollefson; I. Torres; S. Tinoco; T. N. Ukwatta; J. F. Valdés Galicia; P. Vanegas; A. Vázquez; L. Villaseñor; W. Wall; T. Weisgarber; S. Westerhoff; I. G. Wisher; J. Wood; G. B. Yodh; P. W. Younk; D. Zaborov; A. Zepeda; H. Zhou

doi:10.1016/j.astropartphys.2014.08.004

VAMOS: A pathfinder for the HAWC gamma-ray observatory

A. U. Abeysekara, R. Alfaro, C. Alvarez, J. D. Álvarez, F. Ángeles, R. Arceo, J. C. Arteaga-Velázquez, A. Avila-Aroche, H. A. Ayala Solares, C. Badillo, A. S. Barber, B. M. Baughman, N. Bautista-Elivar, J. Becerra Gonzalez, E. Belmont, E. Benítez, S. Y. Benzvi, D. Berley, A. Bernal, M. Bonilla RosalesJ. Braun, R. A. Caballero-Lopez, K. S. Caballero-Mora, I. Cabrera, A. Carramiñana, L. Castañeda-Martínez, M. Castillo, U. Cotti, J. Cotzomi, E. De La Fuente, C. De León, T. Deyoung, A. Diaz-Azuara, L. Diaz-Cruz, R. Diaz Hernandez, J. C. Díaz-Vélez, B. L. Dingus, D. Dultzin, M. A. Duvernois, R. W. Ellsworth, A. Fernandez, D. W. Fiorino, N. Fraija, A. Galindo, G. García-Torales, F. Garfias, A. González, L. X. González, M. M. González, J. A. Goodman, V. Grabski, M. Gussert, C. Guzmán-Cerón, Z. Hampel-Arias, J. P. Harding, L. Hernández-Cervantes, C. M. Hui, P. Hüntemeyer, A. Imran, A. Iriarte, P. Karn, D. Kieda, G. J. Kunde, R. Langarica, A. Lara, G. Lara, R. J. Lauer, W. H. Lee, D. Lennarz, H. León Vargas, E. C. Linares, J. T. Linnemann, M. Longo, R. Luna-Garcia, A. Marinelli, L. A. Martínez, H. Martínez, O. Martínez, J. Martínez-Castro, M. Martos, J. A.J. Matthews, J. McEnery, E. Mendoza Torres, P. Miranda-Romagnoli, E. Moreno, M. Mostafá, J. Nava, L. Nellen, M. Newbold, R. Noriega-Papaqui, T. Oceguera-Becerra, D. P. Page, B. Patricelli, R. Pelayo, E. G. Pérez-Pérez, J. Pretz, I. Ramírez, A. Rentería, C. Rivière, D. Rosa-González, F. Ruiz-Sala, E. L. Ruiz-Velasco, J. Ryan, J. R. Sacahui, H. Salazar, F. Salesa, A. Sandoval, E. Santos, M. Schneider, S. Silich, G. Sinnis, A. J. Smith, K. Sparks Woodle, R. W. Springer, F. Suarez, I. Taboada, A. Tepe, P. A. Toale, K. Tollefson, I. Torres, S. Tinoco, T. N. Ukwatta, J. F. Valdés Galicia, P. Vanegas, A. Vázquez, L. Villaseñor, W. Wall, T. Weisgarber, S. Westerhoff, I. G. Wisher, J. Wood, G. B. Yodh, P. W. Younk, D. Zaborov, A. Zepeda, H. Zhou

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

10 Citas (Scopus)

Resumen

VAMOS¹ was a prototype detector built in 2011 at an altitude of 4100 m 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 30 GeV, for long gamma-ray bursts GRB111016B and GRB120328B.

Idioma original	Inglés
Páginas (desde-hasta)	125-133
Número de páginas	9
Publicación	Astroparticle Physics
Volumen	62
DOI	https://doi.org/10.1016/j.astropartphys.2014.08.004
Estado	Publicada - mar. 2015

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10.1016/j.astropartphys.2014.08.004

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Abeysekara, A. U., Alfaro, R., Alvarez, C., Álvarez, J. D., Ángeles, F., Arceo, R., Arteaga-Velázquez, J. C., Avila-Aroche, A., Ayala Solares, H. A., Badillo, C., Barber, A. S., Baughman, B. M., Bautista-Elivar, N., Becerra Gonzalez, J., Belmont, E., Benítez, E., Benzvi, S. Y., Berley, D., Bernal, A., ... Zhou, H. (2015). VAMOS: A pathfinder for the HAWC gamma-ray observatory. Astroparticle Physics, 62, 125-133. https://doi.org/10.1016/j.astropartphys.2014.08.004

@article{149d60b1d80741699169b5bbe8398f3d,

title = "VAMOS: A pathfinder for the HAWC gamma-ray observatory",

abstract = "VAMOS1 was a prototype detector built in 2011 at an altitude of 4100 m 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 30 GeV, for long gamma-ray bursts GRB111016B and GRB120328B.",

keywords = "Detector prototype, Scientific verification, TeV cosmic rays",

author = "Abeysekara, {A. U.} and R. Alfaro and C. Alvarez and {\'A}lvarez, {J. D.} and F. {\'A}ngeles and R. Arceo and Arteaga-Vel{\'a}zquez, {J. C.} and A. Avila-Aroche and {Ayala Solares}, {H. A.} and C. Badillo and Barber, {A. S.} and Baughman, {B. M.} and N. Bautista-Elivar and {Becerra Gonzalez}, J. and E. Belmont and E. Ben{\'i}tez and Benzvi, {S. Y.} and D. Berley and A. Bernal and {Bonilla Rosales}, M. and J. Braun and Caballero-Lopez, {R. A.} and Caballero-Mora, {K. S.} and I. Cabrera and A. Carrami{\~n}ana and L. Casta{\~n}eda-Mart{\'i}nez and M. Castillo and U. Cotti and J. Cotzomi and {De La Fuente}, E. and {De Le{\'o}n}, C. and T. Deyoung and A. Diaz-Azuara and L. Diaz-Cruz and {Diaz Hernandez}, R. and D{\'i}az-V{\'e}lez, {J. C.} and Dingus, {B. L.} and D. Dultzin and Duvernois, {M. A.} and Ellsworth, {R. W.} and A. Fernandez and Fiorino, {D. W.} and N. Fraija and A. Galindo and G. Garc{\'i}a-Torales and F. Garfias and A. Gonz{\'a}lez and Gonz{\'a}lez, {L. X.} and Gonz{\'a}lez, {M. M.} and Goodman, {J. A.} and V. Grabski and M. Gussert and C. Guzm{\'a}n-Cer{\'o}n and Z. Hampel-Arias and Harding, {J. P.} and L. Hern{\'a}ndez-Cervantes and Hui, {C. M.} and P. H{\"u}ntemeyer and A. Imran and A. Iriarte and P. Karn and D. Kieda and Kunde, {G. J.} and R. Langarica and A. Lara and G. Lara and Lauer, {R. J.} and Lee, {W. H.} and D. Lennarz and {Le{\'o}n Vargas}, H. and Linares, {E. C.} and Linnemann, {J. T.} and M. Longo and R. Luna-Garcia and A. Marinelli and Mart{\'i}nez, {L. A.} and H. Mart{\'i}nez and O. Mart{\'i}nez and J. Mart{\'i}nez-Castro and M. Martos and Matthews, {J. A.J.} and J. McEnery and {Mendoza Torres}, E. and P. Miranda-Romagnoli and E. Moreno and M. Mostaf{\'a} and J. Nava and L. Nellen and M. Newbold and R. Noriega-Papaqui and T. Oceguera-Becerra and Page, {D. P.} and B. Patricelli and R. Pelayo and P{\'e}rez-P{\'e}rez, {E. G.} and J. Pretz and I. Ram{\'i}rez and A. Renter{\'i}a and C. Rivi{\`e}re and D. Rosa-Gonz{\'a}lez and F. Ruiz-Sala and Ruiz-Velasco, {E. L.} and J. Ryan and Sacahui, {J. R.} and H. Salazar and F. Salesa and A. Sandoval and E. Santos and M. Schneider and S. Silich and G. Sinnis and Smith, {A. J.} and {Sparks Woodle}, K. and Springer, {R. W.} and F. Suarez and I. Taboada and A. Tepe and Toale, {P. A.} and K. Tollefson and I. Torres and S. Tinoco and Ukwatta, {T. N.} and {Vald{\'e}s Galicia}, {J. F.} and P. Vanegas and A. V{\'a}zquez and L. Villase{\~n}or and W. Wall and T. Weisgarber and S. Westerhoff and Wisher, {I. G.} and J. Wood and Yodh, {G. B.} and Younk, {P. W.} and D. Zaborov and A. Zepeda and H. Zhou",

year = "2015",

month = mar,

doi = "10.1016/j.astropartphys.2014.08.004",

language = "Ingl{\'e}s",

volume = "62",

pages = "125--133",

journal = "Astroparticle Physics",

issn = "0927-6505",

}

Abeysekara, AU, Alfaro, R, Alvarez, C, Álvarez, JD, Ángeles, F, Arceo, R, Arteaga-Velázquez, JC, Avila-Aroche, A, Ayala Solares, HA, Badillo, C, Barber, AS, Baughman, BM, Bautista-Elivar, N, Becerra Gonzalez, J, Belmont, E, Benítez, E, Benzvi, SY, Berley, D, Bernal, A, Bonilla Rosales, M, Braun, J, Caballero-Lopez, RA, Caballero-Mora, KS, Cabrera, I, Carramiñana, A, Castañeda-Martínez, L, Castillo, M, Cotti, U, Cotzomi, J, De La Fuente, E, De León, C, Deyoung, T, Diaz-Azuara, A, Diaz-Cruz, L, Diaz Hernandez, R, Díaz-Vélez, JC, Dingus, BL, Dultzin, D, Duvernois, MA, Ellsworth, RW, Fernandez, A, Fiorino, DW, Fraija, N, Galindo, A, García-Torales, G, Garfias, F, González, A, González, LX, González, MM, Goodman, JA, Grabski, V, Gussert, M, Guzmán-Cerón, C, Hampel-Arias, Z, Harding, JP, Hernández-Cervantes, L, Hui, CM, Hüntemeyer, P, Imran, A, Iriarte, A, Karn, P, Kieda, D, Kunde, GJ, Langarica, R, Lara, A, Lara, G, Lauer, RJ, Lee, WH, Lennarz, D, León Vargas, H, Linares, EC, Linnemann, JT, Longo, M, Luna-Garcia, R, Marinelli, A, Martínez, LA, Martínez, H, Martínez, O, Martínez-Castro, J, Martos, M, Matthews, JAJ, McEnery, J, Mendoza Torres, E, Miranda-Romagnoli, P, Moreno, E, Mostafá, M, Nava, J, Nellen, L, Newbold, M, Noriega-Papaqui, R, Oceguera-Becerra, T, Page, DP, Patricelli, B, Pelayo, R, Pérez-Pérez, EG, Pretz, J, Ramírez, I, Rentería, A, Rivière, C, Rosa-González, D, Ruiz-Sala, F, Ruiz-Velasco, EL, Ryan, J, Sacahui, JR, Salazar, H, Salesa, F, Sandoval, A, Santos, E, Schneider, M, Silich, S, Sinnis, G, Smith, AJ, Sparks Woodle, K, Springer, RW, Suarez, F, Taboada, I, Tepe, A, Toale, PA, Tollefson, K, Torres, I, Tinoco, S, Ukwatta, TN, Valdés Galicia, JF, Vanegas, P, Vázquez, A, Villaseñor, L, Wall, W, Weisgarber, T, Westerhoff, S, Wisher, IG, Wood, J, Yodh, GB, Younk, PW, Zaborov, D, Zepeda, A & Zhou, H 2015, 'VAMOS: A pathfinder for the HAWC gamma-ray observatory', Astroparticle Physics, vol. 62, pp. 125-133. https://doi.org/10.1016/j.astropartphys.2014.08.004

TY - JOUR

T1 - VAMOS

T2 - A pathfinder for the HAWC gamma-ray observatory

AU - Abeysekara, A. U.

AU - Alfaro, R.

AU - Alvarez, C.

AU - Álvarez, J. D.

AU - Ángeles, F.

AU - Arceo, R.

AU - Arteaga-Velázquez, J. C.

AU - Avila-Aroche, A.

AU - Ayala Solares, H. A.

AU - Badillo, C.

AU - Barber, A. S.

AU - Baughman, B. M.

AU - Bautista-Elivar, N.

AU - Becerra Gonzalez, J.

AU - Belmont, E.

AU - Benítez, E.

AU - Benzvi, S. Y.

AU - Berley, D.

AU - Bernal, A.

AU - Bonilla Rosales, M.

AU - Braun, J.

AU - Caballero-Lopez, R. A.

AU - Caballero-Mora, K. S.

AU - Cabrera, I.

AU - Carramiñana, A.

AU - Castañeda-Martínez, L.

AU - Castillo, M.

AU - Cotti, U.

AU - Cotzomi, J.

AU - De La Fuente, E.

AU - De León, C.

AU - Deyoung, T.

AU - Diaz-Azuara, A.

AU - Diaz-Cruz, L.

AU - Diaz Hernandez, R.

AU - Díaz-Vélez, J. C.

AU - Dingus, B. L.

AU - Dultzin, D.

AU - Duvernois, M. A.

AU - Ellsworth, R. W.

AU - Fernandez, A.

AU - Fiorino, D. W.

AU - Fraija, N.

AU - Galindo, A.

AU - García-Torales, G.

AU - Garfias, F.

AU - González, A.

AU - González, L. X.

AU - González, M. M.

AU - Goodman, J. A.

AU - Grabski, V.

AU - Gussert, M.

AU - Guzmán-Cerón, C.

AU - Hampel-Arias, Z.

AU - Harding, J. P.

AU - Hernández-Cervantes, L.

AU - Hui, C. M.

AU - Hüntemeyer, P.

AU - Imran, A.

AU - Iriarte, A.

AU - Karn, P.

AU - Kieda, D.

AU - Kunde, G. J.

AU - Langarica, R.

AU - Lara, A.

AU - Lara, G.

AU - Lauer, R. J.

AU - Lee, W. H.

AU - Lennarz, D.

AU - León Vargas, H.

AU - Linares, E. C.

AU - Linnemann, J. T.

AU - Longo, M.

AU - Luna-Garcia, R.

AU - Marinelli, A.

AU - Martínez, L. A.

AU - Martínez, H.

AU - Martínez, O.

AU - Martínez-Castro, J.

AU - Martos, M.

AU - Matthews, J. A.J.

AU - McEnery, J.

AU - Mendoza Torres, E.

AU - Miranda-Romagnoli, P.

AU - Moreno, E.

AU - Mostafá, M.

AU - Nava, J.

AU - Nellen, L.

AU - Newbold, M.

AU - Noriega-Papaqui, R.

AU - Oceguera-Becerra, T.

AU - Page, D. P.

AU - Patricelli, B.

AU - Pelayo, R.

AU - Pérez-Pérez, E. G.

AU - Pretz, J.

AU - Ramírez, I.

AU - Rentería, A.

AU - Rivière, C.

AU - Rosa-González, D.

AU - Ruiz-Sala, F.

AU - Ruiz-Velasco, E. L.

AU - Ryan, J.

AU - Sacahui, J. R.

AU - Salazar, H.

AU - Salesa, F.

AU - Sandoval, A.

AU - Santos, E.

AU - Schneider, M.

AU - Silich, S.

AU - Sinnis, G.

AU - Smith, A. J.

AU - Sparks Woodle, K.

AU - Springer, R. W.

AU - Suarez, F.

AU - Taboada, I.

AU - Tepe, A.

AU - Toale, P. A.

AU - Tollefson, K.

AU - Torres, I.

AU - Tinoco, S.

AU - Ukwatta, T. N.

AU - Valdés Galicia, J. F.

AU - Vanegas, P.

AU - Vázquez, A.

AU - Villaseñor, L.

AU - Wall, W.

AU - Weisgarber, T.

AU - Westerhoff, S.

AU - Wisher, I. G.

AU - Wood, J.

AU - Yodh, G. B.

AU - Younk, P. W.

AU - Zaborov, D.

AU - Zepeda, A.

AU - Zhou, H.

PY - 2015/3

Y1 - 2015/3

N2 - VAMOS1 was a prototype detector built in 2011 at an altitude of 4100 m 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 30 GeV, for long gamma-ray bursts GRB111016B and GRB120328B.

AB - VAMOS1 was a prototype detector built in 2011 at an altitude of 4100 m 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 30 GeV, for long gamma-ray bursts GRB111016B and GRB120328B.

KW - Detector prototype

KW - Scientific verification

KW - TeV cosmic rays

UR - http://www.scopus.com/inward/record.url?scp=84919770147&partnerID=8YFLogxK

U2 - 10.1016/j.astropartphys.2014.08.004

DO - 10.1016/j.astropartphys.2014.08.004

M3 - Artículo

SN - 0927-6505

VL - 62

SP - 125

EP - 133

JO - Astroparticle Physics

JF - Astroparticle Physics

ER -

VAMOS: A pathfinder for the HAWC gamma-ray observatory

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