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The Water Cherenkov Detector Array (WCDA) is a major component of the LargeHigh Altitude Air Shower Array Observatory (LHAASO), a new generationcosmic-ray experiment with unprecedented sensitivity, currently underconstruction. The WCDA is aimed at the study of TeV $\gamma$-rays. In order toevaluate the prospects of searching for TeV $\gamma$-ray sources with the WCDA,we present in this paper a projection for the one-year sensitivity of the WCDAto TeV $\gamma$-ray sources from TeVCat (footnote: http://tevcat.uchicago.edu)using an all-sky approach. Out of 128 TeVCat sources observable to the WCDA upto a zenith angle of $45^\circ$, we estimate that 42 would be detectable forone year of observations at a median energy of 1 TeV. Most of them are Galacticsources, and the extragalactic sources are Active Galactic Nuclei (AGN).

Prospects for a Multi-TeV Gamma-ray Sky Survey with the LHAASO Water Cherenkov Detector Array