On the sensitivity of the HAWC observatory to gamma-ray bursts

A. U. Abeysekara; J. A. Aguilar; S. Aguilar; R. Alfaro; E. Almaraz; C. Álvarez; J. De D. Álvarez-Romero; M. Álvarez; R. Arceo; J. C. Arteaga-Velázquez; C. Badillo; A. Barber; B. M. Baughman; N. Bautista-Elivar; E. Belmont; E. Benítez; S. Y. Benzvi; D. Berley; A. Bernal; E. Bonamente; J. Braun; R. Caballero-Lopez; I. Cabrera; A. Carramiñana; L. Carrasco; M. Castillo; L. Chambers; R. Conde; P. Condreay; U. Cotti; J. Cotzomi; J. C. D'Olivo; E. De La Fuente; C. De León; S. Delay; D. Delepine; T. Deyoung; L. Diaz; L. Diaz-Cruz; B. L. Dingus; M. A. Duvernois; D. Edmunds; R. W. Ellsworth; B. Fick; D. W. Fiorino; A. Flandes; N. I. Fraija; A. Galindo; J. L. García-Luna; G. García-Torales; F. Garfias; L. X. González; M. M. González; J. A. Goodman; V. Grabski; M. Gussert; C. Guzmán-Ceron; Z. Hampel-Arias; T. Harris; E. Hays; L. Hernandez-Cervantes; P. H. Hüntemeyer; A. Imran; A. Iriarte; J. J. Jimenez; P. Karn; N. Kelley-Hoskins; D. Kieda; R. Langarica; A. Lara; R. Lauer; W. H. Lee; E. C. Linares; J. T. Linnemann; M. Longo; R. Luna-García; H. Martínez; J. Martínez; L. A. Martínez; O. Martínez; J. Martínez-Castro; M. Martos; J. Matthews; J. E. McEnery; G. Medina-Tanco; J. E. Mendoza-Torres; P. A. Miranda-Romagnoli; T. Montaruli; E. Moreno; M. Mostafa; M. Napsuciale; J. Nava; L. Nellen; M. Newbold; R. Noriega-Papaqui; T. Oceguera-Becerra; A. Olmos Tapia; V. Orozco; V. Pérez; E. G. Pérez-Pérez; J. S. Perkins; J. Pretz; C. Ramirez; I. Ramírez; D. Rebello; A. Rentería; J. Reyes; D. Rosa-González; A. Rosado; J. M. Ryan; J. R. Sacahui; H. Salazar; F. Salesa; A. Sandoval; E. Santos; M. Schneider; A. Shoup; S. Silich; G. Sinnis; A. J. Smith; K. Sparks; W. Springer; F. Suárez; N. Suarez; I. Taboada; A. F. Tellez; G. Tenorio-Tagle; A. Tepe; P. A. Toale; K. Tollefson; I. Torres; T. N. Ukwatta; J. Valdes-Galicia; P. Vanegas; V. Vasileiou; O. Vázquez; X. Vázquez; L. Villaseñor; W. Wall; J. S. Walters; D. Warner; S. Westerhoff; I. G. Wisher; J. Wood; G. B. Yodh; D. Zaborov; A. Zepeda

doi:10.1016/j.astropartphys.2012.02.001

On the sensitivity of the HAWC observatory to gamma-ray bursts

A. U. Abeysekara, J. A. Aguilar, S. Aguilar, R. Alfaro, E. Almaraz, C. Álvarez, J. De D. Álvarez-Romero, M. Álvarez, R. Arceo, J. C. Arteaga-Velázquez, C. Badillo, A. Barber, B. M. Baughman, N. Bautista-Elivar, E. Belmont, E. Benítez, S. Y. Benzvi, D. Berley, A. Bernal, E. BonamenteJ. Braun, R. Caballero-Lopez, I. Cabrera, A. Carramiñana, L. Carrasco, M. Castillo, L. Chambers, R. Conde, P. Condreay, U. Cotti, J. Cotzomi, J. C. D'Olivo, E. De La Fuente, C. De León, S. Delay, D. Delepine, T. Deyoung, L. Diaz, L. Diaz-Cruz, B. L. Dingus, M. A. Duvernois, D. Edmunds, R. W. Ellsworth, B. Fick, D. W. Fiorino, A. Flandes, N. I. Fraija, A. Galindo, J. L. García-Luna, G. García-Torales, F. Garfias, L. X. González, M. M. González, J. A. Goodman, V. Grabski, M. Gussert, C. Guzmán-Ceron, Z. Hampel-Arias, T. Harris, E. Hays, L. Hernandez-Cervantes, P. H. Hüntemeyer, A. Imran, A. Iriarte, J. J. Jimenez, P. Karn, N. Kelley-Hoskins, D. Kieda, R. Langarica, A. Lara, R. Lauer, W. H. Lee, E. C. Linares, J. T. Linnemann, M. Longo, R. Luna-García, H. Martínez, J. Martínez, L. A. Martínez, O. Martínez, J. Martínez-Castro, M. Martos, J. Matthews, J. E. McEnery, G. Medina-Tanco, J. E. Mendoza-Torres, P. A. Miranda-Romagnoli, T. Montaruli, E. Moreno, M. Mostafa, M. Napsuciale, J. Nava, L. Nellen, M. Newbold, R. Noriega-Papaqui, T. Oceguera-Becerra, A. Olmos Tapia, V. Orozco, V. Pérez, E. G. Pérez-Pérez, J. S. Perkins, J. Pretz, C. Ramirez, I. Ramírez, D. Rebello, A. Rentería, J. Reyes, D. Rosa-González, A. Rosado, J. M. Ryan, J. R. Sacahui, H. Salazar, F. Salesa, A. Sandoval, E. Santos, M. Schneider, A. Shoup, S. Silich, G. Sinnis, A. J. Smith, K. Sparks, W. Springer, F. Suárez, N. Suarez, I. Taboada, A. F. Tellez, G. Tenorio-Tagle, A. Tepe, P. A. Toale, K. Tollefson, I. Torres, T. N. Ukwatta, J. Valdes-Galicia, P. Vanegas, V. Vasileiou, O. Vázquez, X. Vázquez, L. Villaseñor, W. Wall, J. S. Walters, D. Warner, S. Westerhoff, I. G. Wisher, J. Wood, G. B. Yodh, D. Zaborov, A. Zepeda

Centro de Investigación en Computación (CIC)

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116 Scopus citations

Abstract

We present the sensitivity of HAWC to gamma ray bursts (GRBs). HAWC is a very high-energy gamma-ray observatory currently under construction in Mexico at an altitude of 4100 m. It will observe atmospheric air showers via the water Cherenkov method. HAWC will consist of 300 large water tanks instrumented with 4 photomultipliers each. HAWC has two data acquisition (DAQ) systems. The main DAQ system reads out coincident signals in the tanks and reconstructs the direction and energy of individual atmospheric showers. The scaler DAQ counts the hits in each photomultiplier tube (PMT) in the detector and searches for a statistical excess over the noise of all PMTs. We show that HAWC has a realistic opportunity to observe the high-energy power law components of GRBs that extend at least up to 30 GeV, as it has been observed by Fermi LAT. The two DAQ systems have an energy threshold that is low enough to observe events similar to GRB 090510 and GRB 090902b with the characteristics observed by Fermi LAT. HAWC will provide information about the high-energy spectra of GRBs which in turn could help to understanding about e-pair attenuation in GRB jets, extragalactic background light absorption, as well as establishing the highest energy to which GRBs accelerate particles.

Original language	English
Pages (from-to)	641-650
Number of pages	10
Journal	Astroparticle Physics
Volume	35
Issue number	10
DOIs	https://doi.org/10.1016/j.astropartphys.2012.02.001
State	Published - May 2012

Keywords

Gamma ray
Gamma-ray bursts

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10.1016/j.astropartphys.2012.02.001

Cite this

Abeysekara, A. U., Aguilar, J. A., Aguilar, S., Alfaro, R., Almaraz, E., Álvarez, C., Álvarez-Romero, J. D. D., Álvarez, M., Arceo, R., Arteaga-Velázquez, J. C., Badillo, C., Barber, A., Baughman, B. M., Bautista-Elivar, N., Belmont, E., Benítez, E., Benzvi, S. Y., Berley, D., Bernal, A., ... Zepeda, A. (2012). On the sensitivity of the HAWC observatory to gamma-ray bursts. Astroparticle Physics, 35(10), 641-650. https://doi.org/10.1016/j.astropartphys.2012.02.001

@article{c314d0590a004724bc7d00c1f735e26c,

title = "On the sensitivity of the HAWC observatory to gamma-ray bursts",

abstract = "We present the sensitivity of HAWC to gamma ray bursts (GRBs). HAWC is a very high-energy gamma-ray observatory currently under construction in Mexico at an altitude of 4100 m. It will observe atmospheric air showers via the water Cherenkov method. HAWC will consist of 300 large water tanks instrumented with 4 photomultipliers each. HAWC has two data acquisition (DAQ) systems. The main DAQ system reads out coincident signals in the tanks and reconstructs the direction and energy of individual atmospheric showers. The scaler DAQ counts the hits in each photomultiplier tube (PMT) in the detector and searches for a statistical excess over the noise of all PMTs. We show that HAWC has a realistic opportunity to observe the high-energy power law components of GRBs that extend at least up to 30 GeV, as it has been observed by Fermi LAT. The two DAQ systems have an energy threshold that is low enough to observe events similar to GRB 090510 and GRB 090902b with the characteristics observed by Fermi LAT. HAWC will provide information about the high-energy spectra of GRBs which in turn could help to understanding about e-pair attenuation in GRB jets, extragalactic background light absorption, as well as establishing the highest energy to which GRBs accelerate particles.",

keywords = "Gamma ray, Gamma-ray bursts",

author = "Abeysekara, {A. U.} and Aguilar, {J. A.} and S. Aguilar and R. Alfaro and E. Almaraz and C. {\'A}lvarez and {\'A}lvarez-Romero, {J. De D.} and M. {\'A}lvarez and R. Arceo and Arteaga-Vel{\'a}zquez, {J. C.} and C. Badillo and A. Barber and Baughman, {B. M.} and N. Bautista-Elivar and E. Belmont and E. Ben{\'i}tez and Benzvi, {S. Y.} and D. Berley and A. Bernal and E. Bonamente and J. Braun and R. Caballero-Lopez and I. Cabrera and A. Carrami{\~n}ana and L. Carrasco and M. Castillo and L. Chambers and R. Conde and P. Condreay and U. Cotti and J. Cotzomi and D'Olivo, {J. C.} and {De La Fuente}, E. and {De Le{\'o}n}, C. and S. Delay and D. Delepine and T. Deyoung and L. Diaz and L. Diaz-Cruz and Dingus, {B. L.} and Duvernois, {M. A.} and D. Edmunds and Ellsworth, {R. W.} and B. Fick and Fiorino, {D. W.} and A. Flandes and Fraija, {N. I.} and A. Galindo and Garc{\'i}a-Luna, {J. L.} and G. Garc{\'i}a-Torales and F. Garfias 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-Ceron and Z. Hampel-Arias and T. Harris and E. Hays and L. Hernandez-Cervantes and H{\"u}ntemeyer, {P. H.} and A. Imran and A. Iriarte and Jimenez, {J. J.} and P. Karn and N. Kelley-Hoskins and D. Kieda and R. Langarica and A. Lara and R. Lauer and Lee, {W. H.} and Linares, {E. C.} and Linnemann, {J. T.} and M. Longo and R. Luna-Garc{\'i}a and H. Mart{\'i}nez and J. Mart{\'i}nez and Mart{\'i}nez, {L. A.} and O. Mart{\'i}nez and J. Mart{\'i}nez-Castro and M. Martos and J. Matthews and McEnery, {J. E.} and G. Medina-Tanco and Mendoza-Torres, {J. E.} and Miranda-Romagnoli, {P. A.} and T. Montaruli and E. Moreno and M. Mostafa and M. Napsuciale and J. Nava and L. Nellen and M. Newbold and R. Noriega-Papaqui and T. Oceguera-Becerra and {Olmos Tapia}, A. and V. Orozco and V. P{\'e}rez and P{\'e}rez-P{\'e}rez, {E. G.} and Perkins, {J. S.} and J. Pretz and C. Ramirez and I. Ram{\'i}rez and D. Rebello and A. Renter{\'i}a and J. Reyes and D. Rosa-Gonz{\'a}lez and A. Rosado and Ryan, {J. M.} and Sacahui, {J. R.} and H. Salazar and F. Salesa and A. Sandoval and E. Santos and M. Schneider and A. Shoup and S. Silich and G. Sinnis and Smith, {A. J.} and K. Sparks and W. Springer and F. Su{\'a}rez and N. Suarez and I. Taboada and Tellez, {A. F.} and G. Tenorio-Tagle and A. Tepe and Toale, {P. A.} and K. Tollefson and I. Torres and Ukwatta, {T. N.} and J. Valdes-Galicia and P. Vanegas and V. Vasileiou and O. V{\'a}zquez and X. V{\'a}zquez and L. Villase{\~n}or and W. Wall and Walters, {J. S.} and D. Warner and S. Westerhoff and Wisher, {I. G.} and J. Wood and Yodh, {G. B.} and D. Zaborov and A. Zepeda",

note = "Funding Information: This work has been supported by: the National Science Foundation , the US Department of Energy Office of High-Energy Physics , the LDRD program of Los Alamos National Laboratory , Consejo Nacional de Ciencia y Tecnologı´a (grants 55155 , 103520 , 105033 , 105666 , 122331 and 132197 ), Red de Fı´sica de Altas Energı´as, DGAPA-UNAM (grants IN105211 , IN112910 and IN121309 , IN115409 ), VIEP-BUAP (grant 161-EXC-2011 ) and the University of Wisconsin Alumni Research Foundation . ",

year = "2012",

month = may,

doi = "10.1016/j.astropartphys.2012.02.001",

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

volume = "35",

pages = "641--650",

journal = "Astroparticle Physics",

issn = "0927-6505",

number = "10",

}

Abeysekara, AU, Aguilar, JA, Aguilar, S, Alfaro, R, Almaraz, E, Álvarez, C, Álvarez-Romero, JDD, Álvarez, M, Arceo, R, Arteaga-Velázquez, JC, Badillo, C, Barber, A, Baughman, BM, Bautista-Elivar, N, Belmont, E, Benítez, E, Benzvi, SY, Berley, D, Bernal, A, Bonamente, E, Braun, J, Caballero-Lopez, R, Cabrera, I, Carramiñana, A, Carrasco, L, Castillo, M, Chambers, L, Conde, R, Condreay, P, Cotti, U, Cotzomi, J, D'Olivo, JC, De La Fuente, E, De León, C, Delay, S, Delepine, D, Deyoung, T, Diaz, L, Diaz-Cruz, L, Dingus, BL, Duvernois, MA, Edmunds, D, Ellsworth, RW, Fick, B, Fiorino, DW, Flandes, A, Fraija, NI, Galindo, A, García-Luna, JL, García-Torales, G, Garfias, F, González, LX, González, MM, Goodman, JA, Grabski, V, Gussert, M, Guzmán-Ceron, C, Hampel-Arias, Z, Harris, T, Hays, E, Hernandez-Cervantes, L, Hüntemeyer, PH, Imran, A, Iriarte, A, Jimenez, JJ, Karn, P, Kelley-Hoskins, N, Kieda, D, Langarica, R, Lara, A, Lauer, R, Lee, WH, Linares, EC, Linnemann, JT, Longo, M, Luna-García, R, Martínez, H, Martínez, J, Martínez, LA, Martínez, O, Martínez-Castro, J, Martos, M, Matthews, J, McEnery, JE, Medina-Tanco, G, Mendoza-Torres, JE, Miranda-Romagnoli, PA, Montaruli, T, Moreno, E, Mostafa, M, Napsuciale, M, Nava, J, Nellen, L, Newbold, M, Noriega-Papaqui, R, Oceguera-Becerra, T, Olmos Tapia, A, Orozco, V, Pérez, V, Pérez-Pérez, EG, Perkins, JS, Pretz, J, Ramirez, C, Ramírez, I, Rebello, D, Rentería, A, Reyes, J, Rosa-González, D, Rosado, A, Ryan, JM, Sacahui, JR, Salazar, H, Salesa, F, Sandoval, A, Santos, E, Schneider, M, Shoup, A, Silich, S, Sinnis, G, Smith, AJ, Sparks, K, Springer, W, Suárez, F, Suarez, N, Taboada, I, Tellez, AF, Tenorio-Tagle, G, Tepe, A, Toale, PA, Tollefson, K, Torres, I, Ukwatta, TN, Valdes-Galicia, J, Vanegas, P, Vasileiou, V, Vázquez, O, Vázquez, X, Villaseñor, L, Wall, W, Walters, JS, Warner, D, Westerhoff, S, Wisher, IG, Wood, J, Yodh, GB, Zaborov, D & Zepeda, A 2012, 'On the sensitivity of the HAWC observatory to gamma-ray bursts', Astroparticle Physics, vol. 35, no. 10, pp. 641-650. https://doi.org/10.1016/j.astropartphys.2012.02.001

TY - JOUR

T1 - On the sensitivity of the HAWC observatory to gamma-ray bursts

AU - Abeysekara, A. U.

AU - Aguilar, J. A.

AU - Aguilar, S.

AU - Alfaro, R.

AU - Almaraz, E.

AU - Álvarez, C.

AU - Álvarez-Romero, J. De D.

AU - Álvarez, M.

AU - Arceo, R.

AU - Arteaga-Velázquez, J. C.

AU - Badillo, C.

AU - Barber, A.

AU - Baughman, B. M.

AU - Bautista-Elivar, N.

AU - Belmont, E.

AU - Benítez, E.

AU - Benzvi, S. Y.

AU - Berley, D.

AU - Bernal, A.

AU - Bonamente, E.

AU - Braun, J.

AU - Caballero-Lopez, R.

AU - Cabrera, I.

AU - Carramiñana, A.

AU - Carrasco, L.

AU - Castillo, M.

AU - Chambers, L.

AU - Conde, R.

AU - Condreay, P.

AU - Cotti, U.

AU - Cotzomi, J.

AU - D'Olivo, J. C.

AU - De La Fuente, E.

AU - De León, C.

AU - Delay, S.

AU - Delepine, D.

AU - Deyoung, T.

AU - Diaz, L.

AU - Diaz-Cruz, L.

AU - Dingus, B. L.

AU - Duvernois, M. A.

AU - Edmunds, D.

AU - Ellsworth, R. W.

AU - Fick, B.

AU - Fiorino, D. W.

AU - Flandes, A.

AU - Fraija, N. I.

AU - Galindo, A.

AU - García-Luna, J. L.

AU - García-Torales, G.

AU - Garfias, F.

AU - González, L. X.

AU - González, M. M.

AU - Goodman, J. A.

AU - Grabski, V.

AU - Gussert, M.

AU - Guzmán-Ceron, C.

AU - Hampel-Arias, Z.

AU - Harris, T.

AU - Hays, E.

AU - Hernandez-Cervantes, L.

AU - Hüntemeyer, P. H.

AU - Imran, A.

AU - Iriarte, A.

AU - Jimenez, J. J.

AU - Karn, P.

AU - Kelley-Hoskins, N.

AU - Kieda, D.

AU - Langarica, R.

AU - Lara, A.

AU - Lauer, R.

AU - Lee, W. H.

AU - Linares, E. C.

AU - Linnemann, J. T.

AU - Longo, M.

AU - Luna-García, R.

AU - Martínez, H.

AU - Martínez, J.

AU - Martínez, L. A.

AU - Martínez, O.

AU - Martínez-Castro, J.

AU - Martos, M.

AU - Matthews, J.

AU - McEnery, J. E.

AU - Medina-Tanco, G.

AU - Mendoza-Torres, J. E.

AU - Miranda-Romagnoli, P. A.

AU - Montaruli, T.

AU - Moreno, E.

AU - Mostafa, M.

AU - Napsuciale, M.

AU - Nava, J.

AU - Nellen, L.

AU - Newbold, M.

AU - Noriega-Papaqui, R.

AU - Oceguera-Becerra, T.

AU - Olmos Tapia, A.

AU - Orozco, V.

AU - Pérez, V.

AU - Pérez-Pérez, E. G.

AU - Perkins, J. S.

AU - Pretz, J.

AU - Ramirez, C.

AU - Ramírez, I.

AU - Rebello, D.

AU - Rentería, A.

AU - Reyes, J.

AU - Rosa-González, D.

AU - Rosado, A.

AU - Ryan, J. M.

AU - Sacahui, J. R.

AU - Salazar, H.

AU - Salesa, F.

AU - Sandoval, A.

AU - Santos, E.

AU - Schneider, M.

AU - Shoup, A.

AU - Silich, S.

AU - Sinnis, G.

AU - Smith, A. J.

AU - Sparks, K.

AU - Springer, W.

AU - Suárez, F.

AU - Suarez, N.

AU - Taboada, I.

AU - Tellez, A. F.

AU - Tenorio-Tagle, G.

AU - Tepe, A.

AU - Toale, P. A.

AU - Tollefson, K.

AU - Torres, I.

AU - Ukwatta, T. N.

AU - Valdes-Galicia, J.

AU - Vanegas, P.

AU - Vasileiou, V.

AU - Vázquez, O.

AU - Vázquez, X.

AU - Villaseñor, L.

AU - Wall, W.

AU - Walters, J. S.

AU - Warner, D.

AU - Westerhoff, S.

AU - Wisher, I. G.

AU - Wood, J.

AU - Yodh, G. B.

AU - Zaborov, D.

AU - Zepeda, A.

N1 - Funding Information: This work has been supported by: the National Science Foundation , the US Department of Energy Office of High-Energy Physics , the LDRD program of Los Alamos National Laboratory , Consejo Nacional de Ciencia y Tecnologı´a (grants 55155 , 103520 , 105033 , 105666 , 122331 and 132197 ), Red de Fı´sica de Altas Energı´as, DGAPA-UNAM (grants IN105211 , IN112910 and IN121309 , IN115409 ), VIEP-BUAP (grant 161-EXC-2011 ) and the University of Wisconsin Alumni Research Foundation .

PY - 2012/5

Y1 - 2012/5

N2 - We present the sensitivity of HAWC to gamma ray bursts (GRBs). HAWC is a very high-energy gamma-ray observatory currently under construction in Mexico at an altitude of 4100 m. It will observe atmospheric air showers via the water Cherenkov method. HAWC will consist of 300 large water tanks instrumented with 4 photomultipliers each. HAWC has two data acquisition (DAQ) systems. The main DAQ system reads out coincident signals in the tanks and reconstructs the direction and energy of individual atmospheric showers. The scaler DAQ counts the hits in each photomultiplier tube (PMT) in the detector and searches for a statistical excess over the noise of all PMTs. We show that HAWC has a realistic opportunity to observe the high-energy power law components of GRBs that extend at least up to 30 GeV, as it has been observed by Fermi LAT. The two DAQ systems have an energy threshold that is low enough to observe events similar to GRB 090510 and GRB 090902b with the characteristics observed by Fermi LAT. HAWC will provide information about the high-energy spectra of GRBs which in turn could help to understanding about e-pair attenuation in GRB jets, extragalactic background light absorption, as well as establishing the highest energy to which GRBs accelerate particles.

AB - We present the sensitivity of HAWC to gamma ray bursts (GRBs). HAWC is a very high-energy gamma-ray observatory currently under construction in Mexico at an altitude of 4100 m. It will observe atmospheric air showers via the water Cherenkov method. HAWC will consist of 300 large water tanks instrumented with 4 photomultipliers each. HAWC has two data acquisition (DAQ) systems. The main DAQ system reads out coincident signals in the tanks and reconstructs the direction and energy of individual atmospheric showers. The scaler DAQ counts the hits in each photomultiplier tube (PMT) in the detector and searches for a statistical excess over the noise of all PMTs. We show that HAWC has a realistic opportunity to observe the high-energy power law components of GRBs that extend at least up to 30 GeV, as it has been observed by Fermi LAT. The two DAQ systems have an energy threshold that is low enough to observe events similar to GRB 090510 and GRB 090902b with the characteristics observed by Fermi LAT. HAWC will provide information about the high-energy spectra of GRBs which in turn could help to understanding about e-pair attenuation in GRB jets, extragalactic background light absorption, as well as establishing the highest energy to which GRBs accelerate particles.

KW - Gamma ray

KW - Gamma-ray bursts

UR - http://www.scopus.com/inward/record.url?scp=84862811823&partnerID=8YFLogxK

U2 - 10.1016/j.astropartphys.2012.02.001

DO - 10.1016/j.astropartphys.2012.02.001

M3 - Artículo

AN - SCOPUS:84862811823

SN - 0927-6505

VL - 35

SP - 641

EP - 650

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 10

ER -

On the sensitivity of the HAWC observatory to gamma-ray bursts

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