{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:SI6F5OTHFX6UUYMFWFOFFLZIDF","short_pith_number":"pith:SI6F5OTH","schema_version":"1.0","canonical_sha256":"923c5eba672dfd4a6185b15c52af28194a92d48d9a50a3aefca0ce4005f3ca40","source":{"kind":"arxiv","id":"1606.08286","version":2},"attestation_state":"computed","paper":{"title":"The clustering properties of radio-selected AGN and star-forming galaxies up to redshifts z~3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"C. Laigle, H.J. McCracken, M. Brusa, M. Magliocchetti, M. Salvato, O.Ilbert, P. Popesso","submitted_at":"2016-06-27T14:29:25Z","abstract_excerpt":"We present the clustering properties of a complete sample of 968 radio sources detected at 1.4 GHz by the VLA-COSMOS survey with radio fluxes brighter than 0.15 mJy. 92% have redshift determinations from the Laigle et al. (2016) catalogue. Based on their radio-luminosity, these objects have been divided into two populations of 644 AGN and 247 star-forming galaxies. By fixing the slope of the auto-correlation function to gamma=2, we find r_0=11.7^{+1.0}_{-1.1} Mpc for the clustering length of the whole sample, while r_0=11.2^{+2.5}_{-3.3} Mpc and r_0=7.8^{+1.6}_{-2.1} Mpc (r_0=6.8^{+1.4}_{-1.8}"},"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":"1606.08286","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-27T14:29:25Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"382c52edadca6b7447c87ae56dd2a765a930269d72a360dce891364578834950","abstract_canon_sha256":"248bf24ebf730162b004578ee200a22f74586f39601aeff2347bf942c0e4e51b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:57:27.210713Z","signature_b64":"Mdn3vOKjp99hBiy2ekE8Eq00uemu8Y08Y7HhrsQno8qzYp1QFN+RIYUQ+3UUmqVjpxVsNiRLrWgHE4HGMrRuBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"923c5eba672dfd4a6185b15c52af28194a92d48d9a50a3aefca0ce4005f3ca40","last_reissued_at":"2026-05-18T00:57:27.210016Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:57:27.210016Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The clustering properties of radio-selected AGN and star-forming galaxies up to redshifts z~3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"C. Laigle, H.J. McCracken, M. Brusa, M. Magliocchetti, M. Salvato, O.Ilbert, P. Popesso","submitted_at":"2016-06-27T14:29:25Z","abstract_excerpt":"We present the clustering properties of a complete sample of 968 radio sources detected at 1.4 GHz by the VLA-COSMOS survey with radio fluxes brighter than 0.15 mJy. 92% have redshift determinations from the Laigle et al. (2016) catalogue. Based on their radio-luminosity, these objects have been divided into two populations of 644 AGN and 247 star-forming galaxies. By fixing the slope of the auto-correlation function to gamma=2, we find r_0=11.7^{+1.0}_{-1.1} Mpc for the clustering length of the whole sample, while r_0=11.2^{+2.5}_{-3.3} Mpc and r_0=7.8^{+1.6}_{-2.1} Mpc (r_0=6.8^{+1.4}_{-1.8}"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.08286","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1606.08286","created_at":"2026-05-18T00:57:27.210137+00:00"},{"alias_kind":"arxiv_version","alias_value":"1606.08286v2","created_at":"2026-05-18T00:57:27.210137+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1606.08286","created_at":"2026-05-18T00:57:27.210137+00:00"},{"alias_kind":"pith_short_12","alias_value":"SI6F5OTHFX6U","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_16","alias_value":"SI6F5OTHFX6UUYMF","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_8","alias_value":"SI6F5OTH","created_at":"2026-05-18T12:30:44.179134+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/SI6F5OTHFX6UUYMFWFOFFLZIDF","json":"https://pith.science/pith/SI6F5OTHFX6UUYMFWFOFFLZIDF.json","graph_json":"https://pith.science/api/pith-number/SI6F5OTHFX6UUYMFWFOFFLZIDF/graph.json","events_json":"https://pith.science/api/pith-number/SI6F5OTHFX6UUYMFWFOFFLZIDF/events.json","paper":"https://pith.science/paper/SI6F5OTH"},"agent_actions":{"view_html":"https://pith.science/pith/SI6F5OTHFX6UUYMFWFOFFLZIDF","download_json":"https://pith.science/pith/SI6F5OTHFX6UUYMFWFOFFLZIDF.json","view_paper":"https://pith.science/paper/SI6F5OTH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1606.08286&json=true","fetch_graph":"https://pith.science/api/pith-number/SI6F5OTHFX6UUYMFWFOFFLZIDF/graph.json","fetch_events":"https://pith.science/api/pith-number/SI6F5OTHFX6UUYMFWFOFFLZIDF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SI6F5OTHFX6UUYMFWFOFFLZIDF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SI6F5OTHFX6UUYMFWFOFFLZIDF/action/storage_attestation","attest_author":"https://pith.science/pith/SI6F5OTHFX6UUYMFWFOFFLZIDF/action/author_attestation","sign_citation":"https://pith.science/pith/SI6F5OTHFX6UUYMFWFOFFLZIDF/action/citation_signature","submit_replication":"https://pith.science/pith/SI6F5OTHFX6UUYMFWFOFFLZIDF/action/replication_record"}},"created_at":"2026-05-18T00:57:27.210137+00:00","updated_at":"2026-05-18T00:57:27.210137+00:00"}