The high altitudewater Čerenkov (HAWC) TeV gamma ray observatory

for the HAWC Collaboration

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

2 Scopus citations

Abstract

The High Altitude Water Čerenkov observatory is a second generation ground based very high-energy γ-ray detector under construction in Sierra Negra, Puebla, México at an altitude of 4,100m. Higher altitude, improved design and a larger physical size used to reject cosmic ray background, make HAWC 10–20 times more sensitive than its predecessorMilagro. HAWC’s large field of view (~2 sr) and over 90% duty cycle make it ideal to search for several types of TeV astronomical γ-ray sources, diffuse emission, cosmic anisotropy, and transients. Details and status of HAWC at date, and a galactic star formation application are here presented.

Original languageEnglish
Title of host publicationCosmic Rays in Star-Forming Environments - Proceedings of the 2nd Session of the Sant Cugat Forum on Astrophysics
EditorsOlaf Reimer, Diego F. Torres
PublisherSpringer Netherlands
Pages439-446
Number of pages8
ISBN (Print)9783642354090
DOIs
StatePublished - 2013
Event2nd Workshop on cosmic-ray induced phenomenology in star-forming environments, 2012 - Catalonia, Spain
Duration: 16 Apr 201219 Apr 2012

Publication series

NameAstrophysics and Space Science Proceedings
Volume34
ISSN (Print)1570-6591
ISSN (Electronic)1570-6605

Conference

Conference2nd Workshop on cosmic-ray induced phenomenology in star-forming environments, 2012
Country/TerritorySpain
CityCatalonia
Period16/04/1219/04/12

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