{"paper":{"title":"A wide-field K-band survey - II. Galaxy clustering","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"C.M. Baugh, C.S. Frenk, J.P.Gardner, R.M. Sharples (University of Durham)","submitted_at":"1996-08-22T09:57:12Z","abstract_excerpt":"We present the first measurement of the angular correlation function in a $K$-selected galaxy survey, from two fields covering almost 10 square degrees. The angular correlation function at small angles is well described by a $\\theta^{-0.8}$ power law, as for optically selected samples. The clustering amplitude is reduced by a factor of $\\sim 4$ between galaxies with $K<15$ and a fainter magnitude slice with $15<K<16$. This allows us to place constraints upon the redshift distribution of the galaxies and their spatial correlation function. We find no clear evidence for a change in clustering am"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9608142","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"}