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

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dc.creatorYabe, Kiyoto
dc.creatorOhta, Kouji
dc.creatorIwata, Ikuru
dc.creatorSawicki, Marcin
dc.creatorTamura, Naoyuki
dc.creatorAkiyama, Masayuki
dc.creatorAoki, Kentaro
dc.date2008-07-01
dc.date.accessioned2026-07-07T09:47:38Z
dc.date.available2026-07-07T09:47:38Z
dc.descriptionWe present the results of Spectral Energy Distribution (SED) fitting analysis for Lyman Break Galaxies (LBGs) at $z\sim5$ in the GOODS-N and its flanking fields. From the SED fitting for $\sim100$ objects, we found that the stellar masses 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 $z\sim5$, we construct the stellar mass function (SMF) with incompleteness corrections. By integrating down to $10^{8}M_{\odot}$, the cosmic stellar mass density at $z\sim5$ is calculated to be $7\times10^{6}M_{\odot}\textrm{Mpc}^{-3}$.
dc.description2 pages, 1 figure, proceedings of the first Subaru International Conference: "Panoramic Views of Galaxy Formation and Evolution", Hayama, Japan, December 2007
dc.identifierhttps://arxiv.org/abs/0807.0137
dc.identifierhttp://arxiv.org/abs/0807.0137
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/163950
dc.subjectAstrophysics
dc.titleThe Stellar Populations of Lyman Break Galaxies at $z\sim5$
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