Identifying galaxy groups at high redshift from incomplete spectroscopic data – I. The group finder and application to zCOSMOS
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DOI: 10.1093/mnras/staa2816
Abstract: Identifying galaxy groups from redshift surveys of galaxies plays an important role in connecting galaxies with the underlying dark matter distribution. Current and future high-$z$ spectroscopic surveys, usually incomplete in redshift sampling, present both opportunities… read more here.
Keywords: identifying galaxy; group finder; group; galaxy groups ... See more keywords