Sensitivity and status of HAWC

FOR THE HAWC COLLABORATION3.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The High Altitude Water Cherenkov (HAWC) Observatory, under construction at Sierra Negra, Mexico will detect energetic air showers from primary hadrons and gamma rays with energies from 100 GeV to 100 TeV. The first stage of the instrument, HAWC-30, with 10% of the channels deployed has been completed and is performing as expected. We anticipate HAWC-100 will be operational by summer 2013 with the full HAWC Observatory (with 300 detectors) being completed in 2014. HAWC complements existing Imaging Atmospheric Cherenkov Telescopes and the space-based gamma-ray telescopes with its extreme high-energy reach and its large field-of-view (∼2sr). The full HAWC instrument will be used to study particle acceleration in Pulsar Wind Nebulae, Supernova Remnants, Active Galactic Nuclei and Gamma-ray Bursts.

Original languageEnglish (US)
Title of host publicationProceedings of the 33rd International Cosmic Rays Conference, ICRC 2013
PublisherSociedade Brasileira de Fisica
ISBN (Electronic)9788589064293
StatePublished - Jan 1 2013
Event33rd International Cosmic Rays Conference, ICRC 2013 - Rio de Janeiro, Brazil
Duration: Jul 2 2013Jul 9 2013

Publication series

NameProceedings of the 33rd International Cosmic Rays Conference, ICRC 2013
Volume2013-October

Other

Other33rd International Cosmic Rays Conference, ICRC 2013
CountryBrazil
CityRio de Janeiro
Period7/2/137/9/13

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics

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  • Cite this

    FOR THE HAWC COLLABORATION3. (2013). Sensitivity and status of HAWC. In Proceedings of the 33rd International Cosmic Rays Conference, ICRC 2013 (Proceedings of the 33rd International Cosmic Rays Conference, ICRC 2013; Vol. 2013-October). Sociedade Brasileira de Fisica.