{"paper":{"title":"The Canada France Redshift Survey VIII: Evolution of the clustering of galaxies from z~1","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. Crampton, D. Hudon, F. Hammer, L. Tresse, O. Le Fevre, S.J. Lilly","submitted_at":"1995-10-18T16:35:48Z","abstract_excerpt":"We have used the projected two-point correlation function, $w(r_p)$, to investigate the spatial distribution of the 591 galaxies with secure redshifts between $0 \\leq z \\leq 1.3$ in the five CFRS fields.\n The slope of the two-point correlation function for the sample as a whole is $\\gamma=1.64\\pm0.05$, very similar to the local slope, and $\\gamma$ is therefore not strongly evolving with redshift. However, the amplitude of the correlation function decreases strongly with increasing redshift, so that at $z\\approx0.6$ it is a factor of 10 lower (for $q_0=0.5$) than for a similarly-selected local "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9510090","kind":"arxiv","version":2},"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"}