The Water Cherenko. Detecto. Array(WCDA) is a majo. co.p.nent o. the Large High Altitude Air Sho.er Array o.servato.y(LHAASo., a new generatio. co.mic-ray exp.riment with unp.ecedented sensitivity, currently under co....
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The Water Cherenko. Detecto. Array(WCDA) is a majo. co.p.nent o. the Large High Altitude Air Sho.er Array o.servato.y(LHAASo., a new generatio. co.mic-ray exp.riment with unp.ecedented sensitivity, currently under co.structio.. WCDA is aimed at the study o. TeV γ-rays. In o.der to.evaluate the p.o.p.cts o. searching fo. TeV γ-ray so.rces with WCDA, we p.esent a p.o.ectio. o. the o.e-year sensitivity o. WCDA to.TeV γ-ray so.rces fro. TeVCat using an all-sky ap.ro.ch. o.t o. 128 TeVCat so.rces o.servable by WCDA up.to.a zenith angle o. 45°, we estimate that 42 wo.ld be detectable in o.e year o. o.servatio.s at a median energy o. 1 TeV. Mo.t o. them are Galactic so.rces, and the extragalactic so.rces are Active Galactic Nuclei(AGN).
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