{"paper":{"title":"The CNOC2 sample of intermediate redshift galaxy groups - the powerhouse of galaxy evolution","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) University of Waterloo, (3) University of Durham, (4) Observatories of the Carnegie Institution, (5) University of Toronto, A. Oemler Jr (4), Canada, Canada), D. J. Wilman (1), Garching, Germany, J. S. Mulchaey (4), M. L. Balogh (2), Pasadena, R. G. Bower (3), R. G. Carlberg (5) ((1) MPE, UK, USA","submitted_at":"2005-10-04T12:23:52Z","abstract_excerpt":"The evolution of galaxies in groups may have important implications for the global evolution of star formation rate in the Universe, since many processes which operate in groups may suppress star formation, and the fraction of galaxies bound in groups at the present day is as high as ~60%. We present an analysis of our sample of 0.3<=z<=0.55 groups, selected from the CNOC2 redshift survey and supplemented with deep spectroscopy and HST ACS imaging. We find that these groups contain significantly more passive galaxies than the field, with excesses of S0, elliptical and passive spiral galaxy typ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0510077","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}