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The High Altitude Water Cherenkov (HAWC) Observatory is a ground-based TeV gamma-ray observatory in the state of Puebla, Mexico at an altitude of 4100 m. Its 22,000 m$^2$ instrumented area, wide field of view ($\sim$2 sr), and >95% uptime…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Joshua Wood

Gamma-ray bursts (GRBs) are among the most luminous sources in the universe and the nature of their emission up to very high energy is one of the most important open issue connected with the study of these peculiar events. The High Altitude…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Simone Dichiara , Maria Magdalena González , Nissim Fraija , Ibrahim Torres , Ana Delia Becerril , Ruben Alfaro , Dirk Lennarz

The High Altitude Water Cherenkov (HAWC) gamma-ray observatory is a wide field of view (1.8 Sr) and high duty cycle (>95% up-time) detector of unique capabilities for the study of TeV gamma-ray sources. Installed at an altitude of 4100m in…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Alberto Carramiñana

The High Altitude Water Cherenkov Observatory (HAWC) is an air shower array currently under construction in Mexico at an altitude of 4100 m. HAWC will consist of 300 large water tanks covering an area of about 22000 square meters and…

High Energy Astrophysical Phenomena · Physics 2019-08-13 D. Zaborov

In this contribution, the first results of HAWC, searching for VHE gamma-ray emission from gamma-ray bursts (GRBs) reported by $\mathit{Swift}$, are presented. The HAWC gamma-ray observatory is operating in central Mexico at an altitude of…

High Energy Astrophysical Phenomena · Physics 2017-05-02 Dirk Lennarz , Ignacio Taboada

The High Altitude Water Cherenkov (HAWC) is a wide field-of-view gamma-ray observatory sensitive to gamma-rays in the 300 GeV - 100 TeV energy range, located in Mexico at an altitude of 4,100 m above sea level. The detector consists of 300…

High Energy Astrophysical Phenomena · Physics 2017-08-15 Cederik de León , Humberto Salazar , Luis Villaseñor

A new ground-based wide-field extensive air shower array known as the High-Altitude Water Cherenkov (HAWC) Observatory promises a new window to monitoring the $\sim$100 GeV gamma-ray sky with the potential for detecting a high energy…

High Energy Astrophysical Phenomena · Physics 2018-01-08 Joshua Wood

The High Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory was completed this year at a 4100-meter site on the flank of the Sierra Negra volcano in Mexico. HAWC is a water Cherenkov ground array with the capability to distinguish 100…

High Energy Astrophysical Phenomena · Physics 2019-08-13 John Pretz

The High-Altitude Water-Cherenkov (HAWC) experiment is a TeV $\gamma$-ray observatory located \unit[4100]{m} above sea level on the Sierra Negra mountain in Puebla, Mexico. The detector consists of 300 water-filled tanks, each instrumented…

Instrumentation and Methods for Astrophysics · Physics 2017-08-14 Samuel Stephens Marinelli , Jordan Goodman

Detections of very-high-energy (VHE; > 100 GeV) photons from Gamma-ray bursts (GRBs) can provide fundamental information on the involved radiative processes, physical composition of the ejecta and acceleration processes. The High Altitude…

High Energy Astrophysical Phenomena · Physics 2019-08-22 Nissim Fraija , M. Magdalena González

The High altitude Water Cherenkov (HAWC) Observatory has been completed and began full operation in early 2015. Located at an elevation of 4,100 m near the Sierra Negra volcano in the state of Puebla, Mexico, HAWC consists of 300 water…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Robert J. Lauer

The High Altitude Water Cherenkov (HAWC) Gamma-ray Observatory is an extensive air shower detector operating in central Mexico, which has recently completed its first two years of full operations. If for a burst like GRB 130427A at a…

High Energy Astrophysical Phenomena · Physics 2017-08-07 The HAWC collaboration , R. Alfaro , C. Alvarez , J. D. Álvarez , R. Arceo , J. C. Arteaga-Velázquez , D. Avila Rojas , H. A. Ayala Solares , A. S. Barber , N. Bautista-Elivar , A. Becerril , E. Belmont-Moreno , S. Y. BenZvi , A. Bernal , J. Braun , C. Brisbois , K. S. Caballero-Mora , T. Capistrán , A. Carramiñana , S. Casanova , M. Castillo , U. Cotti , J. Cotzomi , S. Coutiño de León , E. de la Fuente , C. De León , T. DeYoung , R. Diaz Hernandez , B. L. Dingus , M. A. DuVernois , J. C. Díaz-Vélez , R. W. Ellsworth , K. Engel , D. W. Fiorino , N. Fraija , J. A. García-González , F. Garfias , M. Gerhardt , A. González Muñoz , M. M. González , J. A. Goodman , Z. Hampel-Arias , J. P. Harding , A. Hernandez-Almada , S. Hernandez , B. Hona , C. M. Hui , P. Hüntemeyer , A. Iriarte , A. Jardin-Blicq , V. Joshi , S. Kaufmann , D. Kieda , R. J. Lauer , W. H. Lee , D. Lennarz , H. León Vargas , J. T. Linnemann , A. L. Longinotti , G. Luis Raya , R. Luna-García , K. Malone , S. S. Marinelli , O. Martinez , I. Martinez-Castellanos , J. Martínez-Castro , H. Martínez-Huerta , J. A. Matthews , P. Miranda-Romagnoli , E. Moreno , M. Mostafá , L. Nellen , M. Newbold , R. Noriega-Papaqui , R. Pelayo , E. G. Pérez-Pérez , J. Pretz , Z. Ren , C. D. Rho , C. Rivière , D. Rosa-González , M. Rosenberg , E. Ruiz-Velasco , H. Salazar , F. Salesa Greus , A. Sandoval , M. Schneider , H. Schoorlemmer , G. Sinnis , A. J. Smith , R. W. Springer , P. Surajbali , I. Taboada , O. Tibolla , K. Tollefson , I. Torres , T. N. Ukwatta , G. Vianello , T. Weisgarber , S. Westerhoff , J. Wood , T. Yapici , P. W. Younk , A. Zepeda , H. Zhou

The High Altitude Water Cherenkov (HAWC) observatory is a large field of view, continuously operated, TeV gamma-ray experiment under construction at 4,100 m a.s.l. in Mexico. The HAWC observatory will have an order of magnitude better…

High Energy Astrophysical Phenomena · Physics 2019-08-21 Miguel Mostafa

The High Altitude Water Cherenkov (HAWC) observatory is an array of large water Cherenkov detectors sensitive to gamma rays and hadronic cosmic rays in the energy band between 100 GeV and 100 TeV. The observatory will be used to measure…

High Energy Astrophysical Phenomena · Physics 2016-08-11 A. U. Abeysekara , 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 , E. Belmont , S. Y. BenZvi , D. Berley , M. Bonilla Rosales , J. Braun , R. A. Caballero-Lopez , A. Carramiñana , M. Castillo , U. Cotti , J. Cotzomi , E. de la Fuente , C. De León , T. DeYoung , R. Diaz Hernandez , J. C. Diaz-Velez , B. L. Dingus , M. A. DuVernois , R. W. Ellsworth , A. Fernandez , D. W. Fiorino , N. Fraija , A. Galindo , J. L. Garcia-Luna , G. Garcia-Torales , F. Garfias , L. X. González , M. M. González , J. A. Goodman , V. Grabski , M. Gussert , Z. Hampel-Arias , C. M. Hui , P. Hüntemeyer , A. Imran , A. Iriarte , P. Karn , D. Kieda , G. J. Kunde , A. Lara , R. J. Lauer , W. H. Lee , D. Lennarz , H. León Vargas , E. C. Linares , J. T. Linnemann , M. Longo , R. Luna-García , A. Marinelli , O. Martinez , J. Martínez-Castro , J. A. J. Matthews , P. Miranda-Romagnoli , E. Moreno , M. Mostafá , J. Nava , L. Nellen , M. Newbold , R. Noriega-Papaqui , T. Oceguera-Becerra , B. Patricelli , R. Pelayo , E. G. Pérez-Pérez , J. Pretz , C. Rivière , D. Rosa-González , H. Salazar , F. Salesa , A. Sandoval , E. Santos , M. Schneider , S. Silich , G. Sinnis , A. J. Smith , K. Sparks , R. W. Springer , I. Taboada , P. A. Toale , K. Tollefson , I. Torres , T. N. Ukwatta , L. Villaseñor , T. Weisgarber , S. Westerhoff , I. G. Wisher , J. Wood , G. B. Yodh , P. W. Younk , D. Zaborov , A. Zepeda , H. Zhou

The High-Altitude Water Cherenkov (HAWC) Observatory was completed and began full opera- tion on March 20, 2015. The detector consists of an array of 300 water tanks, each containing 200 ktons of purified water and instrumented with 4 PMTs.…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 Andrew J. Smith

The observation of Gamma Ray Bursts (GRBs) with very-high-energy (VHE) gamma rays can provide understanding of the particle acceleration mechanisms in GRBs, and can also be used to probe the extra-galactic background light and place…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Ignacio Taboada , Rudy C. Gilmore

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…

High Energy Astrophysical Phenomena · Physics 2012-04-26 HAWC collaboration , 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

The High-Altitude Water Cherenkov (HAWC) observatory is a second-generation continuously operated, wide field-of-view, TeV gamma-ray observatory. The HAWC observatory and its analysis techniques build on experience of the Milagro experiment…

High Energy Astrophysical Phenomena · Physics 2023-04-12 A. U. Abeysekara , A. Albert , R. Alfaro , C. Álvarez , J. D. Álvarez , M. Araya , J. C. Arteaga-Velázquez , K. P. Arunbabu , D. Avila Rojas , H. A. Ayala Solares , R. Babu , A. S. Barber , A. Becerril , E. Belmont-Moreno , S. Y. BenZvi , O. Blanco , J. Braun , C. Brisbois , K. S. Caballero-Mora , J. I. Cabrera Martínez , T. Capistrán , A. Carramiñana , S. Casanova , M. Castillo , O. Chaparro-Amaro , U. Cotti , J. Cotzomi , S. Coutiño de León , E. de la Fuente , C. de León , T. De Young , R. Díaz Hernández , B. L. Dingus , M. A. DuVernois , M. Durocher , J. C. Díaz-Vélez , R. W. Ellsworth , K. Engel , C. Espinoza , K. L. Fan , K. Fang , U. B. Fick , H. Fleischhack , J. L. Flores , N. Fraija , J. A. García-González , G. García-Torales , F. Garfias , G. Giacinti , H. Goksu , M. M. González , A. González-Muñoz , J. A. Goodman , J. P. Harding , E. Hernández , S. Hernández , J. Hinton , B. Hona , D. Huang , F. Hueyotl-Zahuantitla , C. M. Hui , T. B. Humensky , P. Hüntemeyer , A. Iriarte , A. Imran , A. Jardin-Blicq , V. Joshi , S. Kaufmann , D. Kieda , G. J. Kunde , A. Lara , R. Lauer , W. H. Lee , D. Lennarz , H. León Vargas , J. T. Linnemann , A. L. Longinotti , G. Luis-Raya , J. Lundeen , K. Malone , V. Marandon , A. Marinelli , O. Martínez , I. Martínez-Castellanos , J. Martínez-Castro , H. Martínez-Huerta , J. A. Matthews , P. Miranda-Romagnoli , T. Montaruli , J. A. Morales-Soto , E. Moreno , M. Mostafá , A. Nayerhoda , L. Nellen , M. Newbold , M. U. Nisa , R. Noriega-Papaqui , T. Oceguera-Becerra , L. Olivera-Nieto , N. Omodei , A. Peisker , Y. Pérez Araujo , E. G. Pérez-Pérez , E. Ponce , J. Pretz , C. D. Rho , D. Rosa-González , E. Ruiz-Velasco , H. Salazar , D. Salazar-Gallegos , F. Salesa Greus , A. Sandoval , M. Schneider , H. Schoorlemmer , J. Serna-Franco , G. Sinnis , A. J. Smith , Y. Son , K. Sparks Woodle , R. W. Springer , I. Taboada , A. Tepe , O. Tibolla , K. Tollefson , I. Torres , R. Torres-Escobedo , R. Turner , F. Ureña-Mena , T. N. Ukwatta , E. Varela , M. Vargas-Magaña , L. Villaseñor , X. Wang , I. J. Watson , F. Werner , S. Westerhoff , E. Willox , I. Wisher , J. Wood , G. B. Yodh , D. Zaborov , A. Zepeda , H. Zhou

The High-Altitude Water Cherenkov Observatory (HAWC) is a large field of view ($\sim$2sr) instrument sensitive to very-high energy gamma rays ($\sim$0.5-100TeV). It is located in central Mexico (19$^\circ$N) and has a high duty cycle…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Israel Martinez-Castellanos

The High-Altitude Water Cherenkov Gamma Ray Observatory (HAWC) is under construction 4100 meters above sea level at Sierra Negra, Mexico. We describe the design and cabling of the detector, the characterization of the photomultipliers, and…

Instrumentation and Methods for Astrophysics · Physics 2013-10-02 HAWC Collaboration , A. U. Abeysekara , 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 , E. Belmont , S. Y. BenZvi , D. Berley , M. Bonilla Rosales , J. Braun , R. A. Caballero-Lopez , K. S. Caballero-Mora , A. Carramiñana , M. Castillo , U. Cotti , J. Cotzomi , E. de la Fuente , C. De León , T. DeYoung , R. Diaz Hernandez , J. C. Díaz-Vélez , B. L. Dingus , M. A. DuVernois , R. W. Ellsworth , A. Fernandez , D. W. Fiorino , N. Fraija , A. Galindo , F. Garfias , L. X. González , M. M. González , J. A. Goodman , V. Grabski , M. Gussert , Z. Hampel-Arias , C. M. Hui , P. Hüntemeyer , A. Imran , A. Iriarte , P. Karn , D. Kieda , G. J. Kunde , A. 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 , H. Martinez , O. Martinez , J. Martínez-Castro , J. A. J. Matthews , P. Miranda-Romagnoli , E. Moreno , M. Mostafá , J. Nava , L. Nellen , M. Newbold , R. Noriega-Papaqui , T. Oceguera-Becerra , B. Patricelli , R. Pelayo , E. G. Pérez-Pérez , J. Pretz , C. Rivière , D. Rosa-González , H. Salazar , F. Salesa , F. E. Sanchez , A. Sandoval , E. Santos , M. Schneider , S. Silich , G. Sinnis , A. J. Smith , K. Sparks , R. W. Springer , I. Taboada , P. A. Toale , K. Tollefson , I. Torres , T. N. Ukwatta , L. Villaseñor , T. Weisgarber , S. Westerhoff , I. G. Wisher , J. Wood , G. B. Yodh , P. W. Younk , D. Zaborov , A. Zepeda , H. Zhou
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