Status of Water Cerenkov Detector Array of LHAASO project

Chen, Mingjun

doi:10.22323/1.301.0832

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Water Cherenkov Detector Array1

Introduction1

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“…Using the hitting information and coverage, the WCDA becomes very sensitive to VHE gamma-rays and cosmic-rays in the energy range 0.1 TeV-30 TeV, with the advantages of a desirable angular resolution, wide field of view and lower threshold energy. [2]…”

Section: Water Cherenkov Detector Arraymentioning

confidence: 99%

“…LHAASO-WCDA is a ground-based air-shower array with the 78,000 m 2 coverage area, to be constructed at high altitude of 4410 meters a.s.l in Daocheng, Sichuan Province, China [1]. It will focus on surveying the northern sky for steady and transient sources from 0.1 TeV to 30 TeV [2], with the advantages of a desirable angular resolution, wide field of view and low threshold energy.…”

Section: Introductionmentioning

confidence: 99%

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