{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1994:C4L4WWJTPUW7YNTE7KJPTKDIBD","short_pith_number":"pith:C4L4WWJT","schema_version":"1.0","canonical_sha256":"1717cb59337d2dfc3664fa92f9a86808f4329fddc1f71a12feb1525b90598c57","source":{"kind":"arxiv","id":"astro-ph/9403042","version":1},"attestation_state":"computed","paper":{"title":"The Clustering Properties of IRAS Galaxies","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Ben Moore, Carlos Frenk, George Efstathiou, Will Saunders","submitted_at":"1994-03-21T01:42:56Z","abstract_excerpt":"We investigate the clustering of galaxies in the QDOT redshift survey of IRAS galaxies. We find that the redshift space two-point correlation function is well approximated by a power-law of slope -1.11+\\-0.09, with clustering length 3.87+\\-0.32 Mpc/h out to pair separations of 25 Mpc\\h. On scales larger than 40 Mpc/h, the correlation function is consistent with zero. The r.m.s. fluctuation in the count of QDOT galaxies above the Poisson level in spheres of radius 8 Mpc/h is \\sigma_8^{IRAS}=0.58+\\-0.14, showing that fluctuations in the distribution of IRAS galaxies on these scales are smaller t"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"astro-ph/9403042","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1994-03-21T01:42:56Z","cross_cats_sorted":[],"title_canon_sha256":"73f321aca05b6de20878b49248d219750a1735a03630173aa3d4552eea452765","abstract_canon_sha256":"d887978428013adc7c878fba472d578989796c4bc5667d7b601e9cd6006ee711"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:26.246214Z","signature_b64":"uxJ03t51DywexnXor5/v+qD2LyBA7JD7D2/FAJ34iuIJYrFpMxAVuAbiyo+caKpSz8Aa1MH5ZFcsm2ZFJs/cCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1717cb59337d2dfc3664fa92f9a86808f4329fddc1f71a12feb1525b90598c57","last_reissued_at":"2026-05-18T01:40:26.245752Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:26.245752Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Clustering Properties of IRAS Galaxies","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Ben Moore, Carlos Frenk, George Efstathiou, Will Saunders","submitted_at":"1994-03-21T01:42:56Z","abstract_excerpt":"We investigate the clustering of galaxies in the QDOT redshift survey of IRAS galaxies. We find that the redshift space two-point correlation function is well approximated by a power-law of slope -1.11+\\-0.09, with clustering length 3.87+\\-0.32 Mpc/h out to pair separations of 25 Mpc\\h. On scales larger than 40 Mpc/h, the correlation function is consistent with zero. The r.m.s. fluctuation in the count of QDOT galaxies above the Poisson level in spheres of radius 8 Mpc/h is \\sigma_8^{IRAS}=0.58+\\-0.14, showing that fluctuations in the distribution of IRAS galaxies on these scales are smaller t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9403042","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/9403042","created_at":"2026-05-18T01:40:26.245820+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9403042v1","created_at":"2026-05-18T01:40:26.245820+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9403042","created_at":"2026-05-18T01:40:26.245820+00:00"},{"alias_kind":"pith_short_12","alias_value":"C4L4WWJTPUW7","created_at":"2026-05-18T12:25:47.102015+00:00"},{"alias_kind":"pith_short_16","alias_value":"C4L4WWJTPUW7YNTE","created_at":"2026-05-18T12:25:47.102015+00:00"},{"alias_kind":"pith_short_8","alias_value":"C4L4WWJT","created_at":"2026-05-18T12:25:47.102015+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/C4L4WWJTPUW7YNTE7KJPTKDIBD","json":"https://pith.science/pith/C4L4WWJTPUW7YNTE7KJPTKDIBD.json","graph_json":"https://pith.science/api/pith-number/C4L4WWJTPUW7YNTE7KJPTKDIBD/graph.json","events_json":"https://pith.science/api/pith-number/C4L4WWJTPUW7YNTE7KJPTKDIBD/events.json","paper":"https://pith.science/paper/C4L4WWJT"},"agent_actions":{"view_html":"https://pith.science/pith/C4L4WWJTPUW7YNTE7KJPTKDIBD","download_json":"https://pith.science/pith/C4L4WWJTPUW7YNTE7KJPTKDIBD.json","view_paper":"https://pith.science/paper/C4L4WWJT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9403042&json=true","fetch_graph":"https://pith.science/api/pith-number/C4L4WWJTPUW7YNTE7KJPTKDIBD/graph.json","fetch_events":"https://pith.science/api/pith-number/C4L4WWJTPUW7YNTE7KJPTKDIBD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/C4L4WWJTPUW7YNTE7KJPTKDIBD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/C4L4WWJTPUW7YNTE7KJPTKDIBD/action/storage_attestation","attest_author":"https://pith.science/pith/C4L4WWJTPUW7YNTE7KJPTKDIBD/action/author_attestation","sign_citation":"https://pith.science/pith/C4L4WWJTPUW7YNTE7KJPTKDIBD/action/citation_signature","submit_replication":"https://pith.science/pith/C4L4WWJTPUW7YNTE7KJPTKDIBD/action/replication_record"}},"created_at":"2026-05-18T01:40:26.245820+00:00","updated_at":"2026-05-18T01:40:26.245820+00:00"}