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Large Scale Structure in COSMOS: Properties of Galaxies in Filaments

Bahram MOBASHER
(University of California, Riverside)

I present a new study of the large scale structure in the COSMOS field. Using a new technique, we assign a density to each galaxy in the COSMOS field and identify clusters and filamentary structures to z~1.2. Using these, we study properties of galaxies in different environments and their evolution with redshift.


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