Evolution of Star-forming Galaxies seen from Lyman Break Galaxies at $z\sim5$
| dc.creator | Ohta, K. | |
| dc.creator | Yabe, K. | |
| dc.creator | Iwata, I. | |
| dc.creator | Sawicki, M. | |
| dc.creator | Akiyama, M. | |
| dc.creator | Tamura, N. | |
| dc.creator | Aoki, K. | |
| dc.date | 2008-07-01 | |
| dc.date.accessioned | 2026-07-07T09:47:38Z | |
| dc.date.available | 2026-07-07T09:47:38Z | |
| dc.description | Properties of Lyman Break Galaxies at $z\sim5$ are presented and are compared with those at $z\sim 2-3$ LBGs to see evolution of LBGs from $z\sim5$ to $z \sim3-2$. The LBGs at $z\sim5$ are tend to have smaller stellar masses, but they may show large star formation rates and specific star formation rates. | |
| dc.description | 4 pages, 2 figures, proceedings of the first Subaru International Conference: "Panoramic Views of Galaxy Formation and Evolution", Hayama, Japan, December 2007 | |
| dc.identifier | https://arxiv.org/abs/0807.0138 | |
| dc.identifier | http://arxiv.org/abs/0807.0138 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/163951 | |
| dc.subject | Astrophysics | |
| dc.title | Evolution of Star-forming Galaxies seen from Lyman Break Galaxies at $z\sim5$ | |
| dc.type | text |