Clustering Segregation With UV Luminosity in Lyman-Break Galaxies at z~3 and Its Implications

Details Clustering Segregation With UV Luminosity in Lyman-Break Galaxies at z~3 and Its Implications Clustering Segregation With UV Luminosity in Lyman-Break Galaxies at z~3 and Its Implications

2000-12-12

arxiv.org/abs/astro-ph/0012249v2

Astronomy and Astrophysics

Astrophysics

Corrected a few typos and added a reference. 36 pages, 8 figures, Latex, AAS macros, to appear on the Astrophysical Journal

Scientific paper

10.1086/319715

We report on the clustering properties of Lyman-break galaxies (LBGs) at z~3. The correlation length of flux-limited samples of LBGs depends on their rest-frame ultraviolet (UV) luminosity at lambda ~1700 Angstrom, with fainter galaxies being less strongly clustered in space. It decreases by a factor ~3 over the range of limiting magnitudes that we have probed, namely 25

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