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We present the results of Spectral Energy Distribution (SED) fitting analysisfor Lyman Break Galaxies (LBGs) at $z\sim5$ in the GOODS-N and its flankingfields. From the SED fitting for $\sim100$ objects, we found that the stellarmasses range from $10^{8}$ to $10^{11}M_{\odot}$ with a median value of$4\times10^{9}M_{\odot}$. By using the large sample of galaxies at $z\sim5$, weconstruct the stellar mass function (SMF) with incompleteness corrections. Byintegrating down to $10^{8}M_{\odot}$, the cosmic stellar mass density at$z\sim5$ is calculated to be $7\times10^{6}M_{\odot}\textrm{Mpc}^{-3}$.

The Stellar Populations of Lyman Break Galaxies at $z\sim5$