Measuring the Rest-Frame UV Properties and the Number Density of Massive Galaxies at 3<z<4

Details Measuring the Rest-Frame UV Properties and the Number Density of Massive Galaxies at 3<z<4 Measuring the Rest-Frame UV Properties and the Number Density of Massive Galaxies at 3<z<4

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010noao.prop..407m&link_type=abstract

NOAO Proposal ID #2010B-0407

Physics

Scientific paper

One of the most controversial questions regarding the build-up of the stellar content of the universe is when and how the most massive galaxies formed. Recent studies have found that the number density of the most massive galaxies has evolved little from z=4 to z~1.5, contrary to the predictions from galaxy formation models, with the largest disagreement being at 3

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