{"paper":{"title":"Spatial Distribution of Low Surface Brightness Galaxies","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"& G.D. Bothun, H.J. Mo, S.S. McGaugh","submitted_at":"1993-11-01T16:26:00Z","abstract_excerpt":"Using redshift samples, we calculate the cross-correlation functions of LSB galaxies with normal galaxies in complete samples (i.e. CfA and IRAS), which enables us to compare directly the amplitudes and shapes of the correlation functions. For pair separations $r\\gs 2\\mpc$, we find that the shape is in agreement with that of the correlation functions for other galaxies. The amplitudes ($A$) of $\\xiab (r)$ are lower than those of the autocorrelation functions for the CfA and IRAS samples, with $A_{\\rm LSB-CfA}:A_{\\rm CfA-CfA}\\approx 0.4$ and $A_{\\rm LSB-IRAS}:A_{\\rm IRAS-IRAS}\\approx 0.6$. Thes"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9311004","kind":"arxiv","version":3},"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"}