M. Castillo
Benemérita Universidad Autónoma de Puebla
9 Papers
118 Citations
M. Castillo is an academic researcher from Benemérita Universidad Autónoma de Puebla. The author has contributed to research in topics: Observatory & Cherenkov radiation. The author has an hindex of 7, co-authored 9 publications.
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Papers
OBSERVATION OF SMALL-SCALE ANISOTROPY IN THE ARRIVAL DIRECTION DISTRIBUTION OF TeV COSMIC RAYS WITH HAWC
Anushka Udara Abeysekara,Anushka Udara Abeysekara,Ruben Alfaro,C. Alvarez,J. D. Álvarez,R. Arceo,J.C. Arteaga-Velázquez,H. A. Ayala Solares,A. S. Barber,B. M. Baughman,N. Bautista-Elivar,E. Belmont,Segev BenZvi,Segev BenZvi,D. Berley,M. Bonilla Rosales,J. Braun,J. Braun,Karen S. Caballero-Mora,A. Carraminana,M. Castillo,U. Cotti,Jorge Cotzomi,E. De la Fuente,C. De León,Tyce DeYoung,R. Diaz Hernandez,Juan Carlos Diaz-Velez,Brenda Dingus,Michael DuVernois,R. W. Ellsworth,R. W. Ellsworth,D. W. Fiorino,Nissim Illich Fraija,A. Galindo,Fernando Garfias,Maria Magdalena González,J. A. Goodman,M. Gussert,Z. Hampel-Arias,J. P. Harding,Petra Hüntemeyer,C. M. Hui,A. Imran,A. Imran,Arturo Iriarte,P. Karn,P. Karn,David Kieda,Gerd Joachim Kunde,Alejandro Lara,R. J. Lauer,William H. Lee,Dirk Lennarz,H. León Vargas,J. T. Linnemann,M. Longo,R. Luna-Garcia,Kelly Malone,A. Marinelli,S. S. Marinelli,H. Martinez,O. Martinez,Jesús Martínez-Castro,J. A. Matthews,Julie McEnery,E. Mendoza Torres,Pedro Miranda-Romagnoli,E. Moreno,Miguel Mostafa,Lukas Nellen,Michael Newbold,R. Noriega-Papaqui,T. Oceguera-Becerra,T. Oceguera-Becerra,B. Patricelli,Rodrigo Pelayo,E. G. Pérez-Pérez,Jennifer Pretz,C. Rivière,C. Rivière,Daniel Rosa-Gonzalez,E. Ruiz-Velasco,James M. Ryan,Humberto Ibarguen Salazar,F. Salesa Greus,A. Sandoval,Michael Schneider,Gus Sinnis,A. J. Smith,K. Sparks Woodle,R. W. Springer,I. Taboada,P. A. Toale,Kirsten Tollefson,I. Torres,T. N. Ukwatta,T. N. Ukwatta,L. Villaseñor,Thomas Weisgarber,S. Westerhoff,I. G. Wisher,Joshua Wood,G. B. Yodh,P. W. Younk,D. Zaborov,Arnulfo Zepeda,and H. Zhou +107 more
TL;DR: In this article, an analysis of the cosmic-ray arrival direction distribution based on 4.9 × 1010 events recorded between 2013 June and 2014 February shows anisotropy at the 10−4 level on angular scales of about 10°.
Sensitivity of HAWC to high-mass dark matter annihilations
Anushka Udara Abeysekara,R. Alfaro,R. Alfaro,C. Alvarez,J. D. Álvarez,R. Arceo,J.C. Arteaga-Velázquez,H. A. Ayala Solares,A. S. Barber,B. M. Baughman,N. Bautista-Elivar,J. Becerra González,J. Becerra González,E. Belmont,Segev BenZvi,D. Berley,M. Bonilla Rosales,J. Braun,R. A. Caballero-Lopez,Karen S. Caballero-Mora,Alberto Carramiñana,M. Castillo,U. Cotti,Jorge Cotzomi,E. De la Fuente,C. De León,Tyce DeYoung,R. Diaz Hernandez,L. Diaz-Cruz,Juan Carlos Diaz-Velez,Juan Carlos Diaz-Velez,Brenda Dingus,Michael DuVernois,R. W. Ellsworth,R. W. Ellsworth,D. W. Fiorino,Nissim Illich Fraija,A. Galindo,Fernando Garfias,Maria Magdalena González,Maria Magdalena González,J. A. Goodman,Varlen Grabski,M. Gussert,Z. Hampel-Arias,J. P. Harding,C. M. Hui,Petra Hüntemeyer,A. Imran,Arturo Iriarte,P. Karn,David Kieda,Gerd Joachim Kunde,Alejandro Lara,R. J. Lauer,William H. Lee,Dirk Lennarz,H. León Vargas,E. C. Linares,J. T. Linnemann,M. Longo,R. Luna-Garcia,A. Marinelli,H. Martinez,O. Martinez,Jesús Martínez-Castro,J. A.J. Matthews,Julie McEnery,E. Mendoza Torres,Pedro Miranda-Romagnoli,E. Moreno,Miguel Mostafa,L. Nellen,Michael Newbold,R. Noriega-Papaqui,T. Oceguera-Becerra,T. Oceguera-Becerra,B. Patricelli,Rodrigo Pelayo,E. G. Pérez-Pérez,J. Pretz,Colas Rivière,Daniel Rosa-Gonzalez,James M. Ryan,Humberto Ibarguen Salazar,F. Salesa,F. E. Sanchez,A. Sandoval,Michael Schneider,S. Silich,G. Sinnis,A. J. Smith,K. Sparks Woodle,R. W. Springer,I. Taboada,P. A. Toale,K. Tollefson,I. Torres,T. N. Ukwatta,L. Villaseñor,Thomas Weisgarber,S. Westerhoff,I. G. Wisher,Joshua Wood,G. B. Yodh,P. W. Younk,D. Zaborov,A. Zepeda,Hao Zhou,Kevork N. Abazajian +109 more
TL;DR: Abeysekara et al. as discussed by the authors studied the HAWC sensitivity to gamma-ray signatures of high-mass (multi-TeV) dark matter annihilation.
VAMOS: a Pathfinder for the HAWC Gamma-Ray Observatory
Anushka Udara Abeysekara,Ruben 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 González,J. Becerra González,E. Belmont,Erika Benítez,Segev BenZvi,D. Berley,A. Bernal,M. Bonilla Rosales,J. Braun,R. A. Caballero-Lopez,Karen S. Caballero-Mora,I. Cabrera,Alberto Carramiñana,L. Castañeda-Martínez,M. Castillo,Umberto Cotti,Jorge Cotzomi,E. De la Fuente,C. De León,Tyce DeYoung,A. Diaz-Azuara,L. Diaz-Cruz,R. Diaz Hernandez,Juan Carlos Diaz-Velez,Brenda Dingus,Deborah Dultzin,Michael DuVernois,R. W. Ellsworth,R. W. Ellsworth,A. Fernandez,D. W. Fiorino,Nissim Illich Fraija,A. Galindo,Guillermo Garcia-Torales,Fernando Garfias,A. González,Luis Xavier Gonzalez,Maria Magdalena González,J. A. Goodman,Varlen Grabski,M. Gussert,C. Guzmán-Ceron,Z. Hampel-Arias,J. P. Harding,L. Hernandez-Cervantes,C. M. Hui,Petra Hüntemeyer,A. Imran,Arturo Iriarte,P. Karn,David Kieda,Gerd Joachim Kunde,R. Langarica,Alejandro Lara,G. Lara,R. J. Lauer,William H. Lee,Dirk Lennarz,H. León Vargas,E. C. Linares,J. T. Linnemann,M. Longo,R. Luna-Garcia,A. Marinelli,L. A. Martínez,H. Martinez,O. Martinez,Jesús Martínez-Castro,M. Martos,J. A.J. Matthews,Julie McEnery,E. Mendoza Torres,Pedro Miranda-Romagnoli,E. Moreno,Miguel Mostafa,J. Nava,L. Nellen,Michael Newbold,R. Noriega-Papaqui,T. Oceguera-Becerra,Dany Page,B. Patricelli,Rodrigo Pelayo,E. G. Pérez-Pérez,Jennifer Pretz,I. Ramírez,A. Rentería,Colas Rivière,Daniel Rosa-Gonzalez,F. Ruiz-Sala,E. Ruiz-Velasco,James M. Ryan,J. R. Sacahui,Humberto Ibarguen Salazar,F. Salesa,A. Sandoval,Elton J. G. Santos,Michael 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,Ibrahim Torres,S. Tinoco,T. N. Ukwatta,J. F. Valdés Galicia,P. Vanegas,A. Vázquez,L. Villaseñor,W. Wall,Thomas Weisgarber,S. Westerhoff,I. G. Wisher,Joshua Wood,G. B. Yodh,P. W. Younk,D. Zaborov,A. Zepeda,Hao Zhou +137 more
TL;DR: The VAMOS 1 was a prototype detector built in 2011 at an altitude of 4100m a.s.l in the state of Puebla, Mexico as mentioned in this paper, which was used to finalize the design, construction techniques and data acquisition system of the HAWC observatory.
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Simulation of Fano factor at HAWC-30 array
M. Castillo,Humberto Ibarguen Salazar,A Tepe,L. Villaseñor +3 more
- 10 Aug 2012
TL;DR: In this article, the results of simulations where the goal is to get Fano factor in order to simulate the HAWC-30 array sensibility to gamma-ray bursts using the single particle technique.
Study of capabilities of the HAWC observatory to detect GRBs
M. Castillo,Humberto Ibarguen Salazar,L. Villaseñor +2 more
- 01 Apr 2011
TL;DR: In this paper, the authors describe the simulation of atmospheric air showers originated by gamma rays with energies in the 0.1-1 TeV range and study the properties of the secondary particles at a height above level of 4100 m corresponding to the height of the array of water Cherenkov detectors (WCDs) of the HAWC Observatory.