The Galaxy Major Merger Rate at z>3: Constraints on Galaxy Evolution and the LCDM Paradigm

Details The Galaxy Major Merger Rate at z>3: Constraints on Galaxy Evolution and the LCDM Paradigm The Galaxy Major Merger Rate at z>3: Constraints on Galaxy Evolution and the LCDM Paradigm

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11772r&link_type=abstract

HST Proposal ID #11772. Cycle 17

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Scientific paper

We propose to determine the highest redshift portion {33. While galaxy merging is widely regarded as the primary mechanism of galaxy evolution, there are currently no merger studies at z>3. When our results are combined with the wealth of published data at z<1 and our work at 0.5

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