Luminosity dependent evolution of lyman break galaxies from redshift 5 to 3

I. Iwata, K. Ohta, N. Tamura, M. Akiyama, K. Aoki, M. Ando, G. Kiuchi, M. Sawicki

Research output: Contribution to journalArticlepeer-review

Abstract

The development of large ground-based telescopes and sensitive large format detectors, as well as the develepment of various techniques for the selection of high-z galaxies enabled us to construct large samples of galaxies in the early universe, as reported in the many contributions in this proceedings. The next major step for the comprehensive understanding of the galaxy evolution would be to explore the relationship of galaxies selected with different criteria at different epochs and find links between them. In this contribution we present the properties of Lyman break galaxies (LBGs) at z∼5 obtained by deep and wide blank field surveys, and through the comparison with samples at lower redshift ranges we discuss the evolution of star-forming galaxies in the early universe.

Original languageEnglish
Pages (from-to)364-365
Number of pages2
JournalProceedings of the International Astronomical Union
Volume2
Issue numberS235
DOIs
Publication statusPublished - 2006 Aug
Externally publishedYes

Keywords

  • Galaxies: evolution
  • Galaxies: high-redshift
  • Galaxies: starburst

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Luminosity dependent evolution of lyman break galaxies from redshift 5 to 3'. Together they form a unique fingerprint.

Cite this