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The High Altitude Water Cherenkov (HAWC) gamma-ray observatory consists of 300 water Cherenkov detectors and has been fully operational since March 2015 in central Mexico. It detects cosmic- and gamma-ray showers in the TeV energy range.…

Instrumentation and Methods for Astrophysics · Physics 2017-08-15 Vikas Joshi , Armelle Jardin-Blicq

The High Altitude Water Cherenkov (HAWC) observatory is a very high energy gamma-ray detector located in Mexico. In late 2018, the HAWC collaboration completed a major upgrade consisting of the addition of a sparse outrigger array of 345…

Instrumentation and Methods for Astrophysics · Physics 2019-08-22 Vincent Marandon , Armelle Jardin-Blicq , Harm Schoorlemmer

The High Altitude Water Cherenkov (HAWC) high-energy gamma-ray observatory has recently been completed on the slopes of the Sierra Negra volcano in central Mexico. HAWC consists of 300 Water Cherenkov Detectors, each containing 180 m$^3$ of…

Instrumentation and Methods for Astrophysics · Physics 2015-09-16 A. Sandoval

The High Altitude Water Cherenkov (HAWC) high-energy {\gamma}-ray observatory was completed in march 2015 in central Mexico. The detector, consisting of 300 water tanks, is currently being upgraded to improve its performance at Multi-TeV…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 Armelle Jardin-Blicq , Vikas Joshi

The High Altitude Water Cherenkov (HAWC) gamma-ray observatory detects cosmic- and gamma-ray initiated air showers in the TeV energy range using 300 water Cherenkov detectors (WCDs). To improve its sensitivity at the highest energies, HAWC…

Instrumentation and Methods for Astrophysics · Physics 2019-08-20 Vikas Joshi , Harm Schoorlemmer

The High Altitude Water Cherenkov (HAWC) observatory is an air-shower array located in Mexico. It is sensitive to the highest energy photons we detect at the Earth, reaching energies of several tens of TeV. The observatory was completed…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 R. López-Coto

The High Altitude Water Cherenkov (HAWC) gamma-ray observatory is a ground-based air shower array designed to detect Cherenkov light produced in water by secondary particles from atmospheric air showers. In order to improve the sensitivity…

High Energy Astrophysical Phenomena · Physics 2019-09-02 Dezhi Huang

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 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

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 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

The High Altitude Water Cherenkov (HAWC) observatory monitors the gamma-ray sky at energies between 100 GeV and 100 TeV with a wide field of view of $\sim 2$ steradians. A duty cycle of $\sim 90$% allows HAWC to scan two thirds of the sky…

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

The High-Altitude Water Cherenkov (HAWC) Observatory is used for detecting TeV gamma rays. HAWC is operating at 4,100 meters above level sea on the slope of the Sierra Negra Volcano in the State of Puebla, Mexico, and consists of an array…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 T. Capistrán , I. Torres , E. Moreno

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

The High Altitude Water Cherenkov Gamma-Ray Observatory has been accumulating a progressively deeper exposure of the TeV sky since its inauguration in March 2015. Located at geographical latitude $+19^\circ$N, HAWC has been able to perform…

High Energy Astrophysical Phenomena · Physics 2019-08-20 Alberto Carramiñana , Daniel Rosa González , Sara Coutiño de León , Anna Lia Longinotti

The recently completed High Altitude Water Cherenkov (HAWC) gamma-ray observatory has been taking data with a partial array for more than one year and is now operating with >95% duty cycle in its full configuration. With an instantaneous…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Robert J. Lauer , Patrick W. Younk

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) Observatory, located on the slopes of the Sierra Negra volcano in Mexico, began operations in March 2015. Over the past decade, HAWC has enabled the exploration of a broad range of topics in…

High Energy Astrophysical Phenomena · Physics 2025-12-04 Anna Lia Longinotti , HAWC Collaboration

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
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