The Star Formation Rate-Density Relationship at Redshift Three

Details The Star Formation Rate-Density Relationship at Redshift Three The Star Formation Rate-Density Relationship at Redshift Three

2005-03-04

arxiv.org/abs/astro-ph/0503094v2

Astrophys.J. 623 (2005) L75-L79

Astronomy and Astrophysics

Astrophysics

4 pages, 4 figures, accepted for publication in ApJL; minor changes to match the published text

Scientific paper

10.1086/430109

We study the star formation rate (SFR) as a function of environment for UV selected Lyman break galaxies (LBGs) at redshift three. From deep UBVI KPNO 4-m/MOSAIC images, covering a total of 0.90 deg^2, we select 334 LBGs in slices 100 Mpc (co-moving) deep spanning the redshift range 2.9

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