{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:NTFC3LJAXAUXG6PZ5UEA2X65TX","short_pith_number":"pith:NTFC3LJA","schema_version":"1.0","canonical_sha256":"6cca2dad20b8297379f9ed080d5fdd9df0533c72019065368a16c99bbf9091f7","source":{"kind":"arxiv","id":"1607.06097","version":1},"attestation_state":"computed","paper":{"title":"Detection of Baryon Acoustic Oscillation Features in the Large-Scale 3-Point Correlation Function of SDSS BOSS DR12 CMASS Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"An\\v{z}e Slosar, Ashley J. Ross, Chia-Hsun Chuang, Daniel J. Eisenstein, Francisco-Shu Kitaura, Graziano Rossi, H\\'ector Gil-Mar\\'in, Hee-Jong Seo, Joel R. Brownstein, Mariana Vargas-Maga\\~na, Shirley Ho, Will J. Percival, Zachary Slepian","submitted_at":"2016-07-20T20:00:07Z","abstract_excerpt":"We present the large-scale 3-point correlation function (3PCF) of the SDSS DR12 CMASS sample of $777,202$ Luminous Red Galaxies, the largest-ever sample used for a 3PCF or bispectrum measurement. We make the first high-significance ($4.5\\sigma$) detection of Baryon Acoustic Oscillations (BAO) in the 3PCF. Using these acoustic features in the 3PCF as a standard ruler, we measure the distance to $z=0.57$ to $1.7\\%$ precision (statistical plus systematic). We find $D_{\\rm V}= 2024\\pm29\\;{\\rm Mpc\\;(stat)}\\pm20\\;{\\rm Mpc\\;(sys)}$ for our fiducial cosmology (consistent with Planck 2015) and bias mod"},"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":"1607.06097","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-07-20T20:00:07Z","cross_cats_sorted":[],"title_canon_sha256":"a6775bbf11389e900942aeaf953a6a2b6d7de8a88c5acdc36d4eb0a9291c24bd","abstract_canon_sha256":"f05062c16fcdf2128fed70056871d546ec3d5b85471bdd8dc1bdbba445582c90"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:42:07.678999Z","signature_b64":"FZYxof/9lwxZMGaFflrEBg/brh1Q7dJ89r1PsgkQFYfpWRcmxARxUaer6dxvgcg+p8WUV2AvVjO9hG7XVR+zCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6cca2dad20b8297379f9ed080d5fdd9df0533c72019065368a16c99bbf9091f7","last_reissued_at":"2026-05-18T00:42:07.678420Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:42:07.678420Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detection of Baryon Acoustic Oscillation Features in the Large-Scale 3-Point Correlation Function of SDSS BOSS DR12 CMASS Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"An\\v{z}e Slosar, Ashley J. Ross, Chia-Hsun Chuang, Daniel J. Eisenstein, Francisco-Shu Kitaura, Graziano Rossi, H\\'ector Gil-Mar\\'in, Hee-Jong Seo, Joel R. Brownstein, Mariana Vargas-Maga\\~na, Shirley Ho, Will J. Percival, Zachary Slepian","submitted_at":"2016-07-20T20:00:07Z","abstract_excerpt":"We present the large-scale 3-point correlation function (3PCF) of the SDSS DR12 CMASS sample of $777,202$ Luminous Red Galaxies, the largest-ever sample used for a 3PCF or bispectrum measurement. We make the first high-significance ($4.5\\sigma$) detection of Baryon Acoustic Oscillations (BAO) in the 3PCF. Using these acoustic features in the 3PCF as a standard ruler, we measure the distance to $z=0.57$ to $1.7\\%$ precision (statistical plus systematic). We find $D_{\\rm V}= 2024\\pm29\\;{\\rm Mpc\\;(stat)}\\pm20\\;{\\rm Mpc\\;(sys)}$ for our fiducial cosmology (consistent with Planck 2015) and bias mod"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.06097","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":"1607.06097","created_at":"2026-05-18T00:42:07.678509+00:00"},{"alias_kind":"arxiv_version","alias_value":"1607.06097v1","created_at":"2026-05-18T00:42:07.678509+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.06097","created_at":"2026-05-18T00:42:07.678509+00:00"},{"alias_kind":"pith_short_12","alias_value":"NTFC3LJAXAUX","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_16","alias_value":"NTFC3LJAXAUXG6PZ","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_8","alias_value":"NTFC3LJA","created_at":"2026-05-18T12:30:36.002864+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2605.23367","citing_title":"Cosmological constraints from neighbor-density-weighted marked correlation functions","ref_index":43,"is_internal_anchor":true},{"citing_arxiv_id":"2407.03397","citing_title":"No evidence for parity violation in BOSS","ref_index":23,"is_internal_anchor":true},{"citing_arxiv_id":"2408.03036","citing_title":"Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study","ref_index":53,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NTFC3LJAXAUXG6PZ5UEA2X65TX","json":"https://pith.science/pith/NTFC3LJAXAUXG6PZ5UEA2X65TX.json","graph_json":"https://pith.science/api/pith-number/NTFC3LJAXAUXG6PZ5UEA2X65TX/graph.json","events_json":"https://pith.science/api/pith-number/NTFC3LJAXAUXG6PZ5UEA2X65TX/events.json","paper":"https://pith.science/paper/NTFC3LJA"},"agent_actions":{"view_html":"https://pith.science/pith/NTFC3LJAXAUXG6PZ5UEA2X65TX","download_json":"https://pith.science/pith/NTFC3LJAXAUXG6PZ5UEA2X65TX.json","view_paper":"https://pith.science/paper/NTFC3LJA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1607.06097&json=true","fetch_graph":"https://pith.science/api/pith-number/NTFC3LJAXAUXG6PZ5UEA2X65TX/graph.json","fetch_events":"https://pith.science/api/pith-number/NTFC3LJAXAUXG6PZ5UEA2X65TX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NTFC3LJAXAUXG6PZ5UEA2X65TX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NTFC3LJAXAUXG6PZ5UEA2X65TX/action/storage_attestation","attest_author":"https://pith.science/pith/NTFC3LJAXAUXG6PZ5UEA2X65TX/action/author_attestation","sign_citation":"https://pith.science/pith/NTFC3LJAXAUXG6PZ5UEA2X65TX/action/citation_signature","submit_replication":"https://pith.science/pith/NTFC3LJAXAUXG6PZ5UEA2X65TX/action/replication_record"}},"created_at":"2026-05-18T00:42:07.678509+00:00","updated_at":"2026-05-18T00:42:07.678509+00:00"}