The Origin and Evolution of Low-Redshift (z<2) Lyman Alpha Emitting Galaxies

Details The Origin and Evolution of Low-Redshift (z<2) Lyman Alpha Emitting Galaxies The Origin and Evolution of Low-Redshift (z<2) Lyman Alpha Emitting Galaxies

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010noao.prop..437d&link_type=abstract

NOAO Proposal ID #2010B-0437

Physics

Scientific paper

Low luminosity galaxies contribute significantly to the mass and star-formation density of the universe at early epochs. Ly(alpha) emitting galaxies (LAEs) are powerful probes of the low-luminosity end of the luminosity function, and are also used to place constraints on the reionization epoch and the early mass assembly of galaxies. Most LAE studies have focused primarily on high redshifts (z~3-7) where the physical nature and large-scale context of LAEs remain largely unconstrained. In order to remedy this situation, we have begun a survey for LAEs at 1.8

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