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Star Formation and Structure Formation at Redshifts 1 < z < 4

K. L. Adelberger
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Abstract

The advent of 8m-class telescopes has made galaxies at 1 < z < 4 relatively easy to detect and study. This is a brief and incomplete review of some of the recent results to emerge from surveys at these redshifts. After describing different strategies for finding galaxies at z >~ 1, and the differences (and similarities) in the resulting galaxy samples, I summarize what is known about the spatial clustering of star-forming galaxies at z >~ 1. Optically selected galaxies are the main focus of this review, but in the final section I discuss the connection between optical and sub-mm samples, and argue that the majority of the 850 micron background may have been produced by known optically selected populations at high redshift. Among the new results presented are the dust-corrected luminosity function of Lyman-break galaxies at z~3, the estimated contribution to the 850 micron background from optically selected galaxies at 1 = 1.0, sigma_z = 0.10.

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K. L. Adelberger. 1999-12-08. Star Formation and Structure Formation at Redshifts 1 < z < 4. https://arxiv.org/abs/astro-ph/9912153

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