{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:CPTIVIDT53XD4S3BT56KF7DGLP","short_pith_number":"pith:CPTIVIDT","schema_version":"1.0","canonical_sha256":"13e68aa073eeee3e4b619f7ca2fc665bdb64616c69298760e7bd7d9281c91e78","source":{"kind":"arxiv","id":"1607.03147","version":1},"attestation_state":"computed","paper":{"title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Ariel G. Sanchez, Ashley J. Ross, Chia-Hsun Chuang, Claudio DallaVecchia, Daniel J. Eisenstein, Florian Beutler, Francisco Prada, Francisco-Shu Kitaura, Gong-Bo Zhao, Hee-Jong Seo, Jan Niklas Grieb, Jeremy Tinker, Joel R. Brownstein, Lado Samushia, Mariana Vargas-Magana, Martha Lippich, Martin Crocce, Matthew D. Olmstead, Rita Tojeiro, Roman Scoccimarro, Salvador Salazar-Albornoz, Sergio Rodriguez-Torres, Will J. Percival, Yuting Wang","submitted_at":"2016-07-11T20:29:44Z","abstract_excerpt":"We explore the cosmological implications of anisotropic clustering measurements in configuration space of the final galaxy samples from Data Release 12 of the SDSS-III Baryon Oscillation Spectroscopic Survey. We implement a new detailed modelling of the effects of non-linearities, galaxy bias and redshift-space distortions that can be used to extract unbiased cosmological information from our measurements for scales $s \\gtrsim 20\\,h^{-1}{\\rm Mpc}$. We combined the galaxy clustering information from BOSS with the latest cosmic microwave background (CMB) observations and Type Ia supernovae sampl"},"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":"1607.03147","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-07-11T20:29:44Z","cross_cats_sorted":[],"title_canon_sha256":"d01c0d759f657e0153f4b1b3929c8f565076fadc2966f14e4a2a50b32b5cb68e","abstract_canon_sha256":"e13cbada17740e449ab54dba87e4782b0b56fda618a9b33300c9e043f9048543"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:59:24.431736Z","signature_b64":"G0awCDb2zYR4te5nT6EtcOgEpUDclt1gkz3VEIPa4ZfupUTYQPmIeet5GTm8M4cbojvOAMj8FMcer/AyRy/mBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"13e68aa073eeee3e4b619f7ca2fc665bdb64616c69298760e7bd7d9281c91e78","last_reissued_at":"2026-05-18T00:59:24.431067Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:59:24.431067Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Ariel G. Sanchez, Ashley J. Ross, Chia-Hsun Chuang, Claudio DallaVecchia, Daniel J. Eisenstein, Florian Beutler, Francisco Prada, Francisco-Shu Kitaura, Gong-Bo Zhao, Hee-Jong Seo, Jan Niklas Grieb, Jeremy Tinker, Joel R. Brownstein, Lado Samushia, Mariana Vargas-Magana, Martha Lippich, Martin Crocce, Matthew D. Olmstead, Rita Tojeiro, Roman Scoccimarro, Salvador Salazar-Albornoz, Sergio Rodriguez-Torres, Will J. Percival, Yuting Wang","submitted_at":"2016-07-11T20:29:44Z","abstract_excerpt":"We explore the cosmological implications of anisotropic clustering measurements in configuration space of the final galaxy samples from Data Release 12 of the SDSS-III Baryon Oscillation Spectroscopic Survey. We implement a new detailed modelling of the effects of non-linearities, galaxy bias and redshift-space distortions that can be used to extract unbiased cosmological information from our measurements for scales $s \\gtrsim 20\\,h^{-1}{\\rm Mpc}$. We combined the galaxy clustering information from BOSS with the latest cosmic microwave background (CMB) observations and Type Ia supernovae sampl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.03147","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":"1607.03147","created_at":"2026-05-18T00:59:24.431164+00:00"},{"alias_kind":"arxiv_version","alias_value":"1607.03147v1","created_at":"2026-05-18T00:59:24.431164+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.03147","created_at":"2026-05-18T00:59:24.431164+00:00"},{"alias_kind":"pith_short_12","alias_value":"CPTIVIDT53XD","created_at":"2026-05-18T12:30:09.641336+00:00"},{"alias_kind":"pith_short_16","alias_value":"CPTIVIDT53XD4S3B","created_at":"2026-05-18T12:30:09.641336+00:00"},{"alias_kind":"pith_short_8","alias_value":"CPTIVIDT","created_at":"2026-05-18T12:30:09.641336+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2408.03036","citing_title":"Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study","ref_index":74,"is_internal_anchor":true},{"citing_arxiv_id":"2411.12021","citing_title":"DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars","ref_index":39,"is_internal_anchor":true},{"citing_arxiv_id":"2411.12022","citing_title":"DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements","ref_index":25,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CPTIVIDT53XD4S3BT56KF7DGLP","json":"https://pith.science/pith/CPTIVIDT53XD4S3BT56KF7DGLP.json","graph_json":"https://pith.science/api/pith-number/CPTIVIDT53XD4S3BT56KF7DGLP/graph.json","events_json":"https://pith.science/api/pith-number/CPTIVIDT53XD4S3BT56KF7DGLP/events.json","paper":"https://pith.science/paper/CPTIVIDT"},"agent_actions":{"view_html":"https://pith.science/pith/CPTIVIDT53XD4S3BT56KF7DGLP","download_json":"https://pith.science/pith/CPTIVIDT53XD4S3BT56KF7DGLP.json","view_paper":"https://pith.science/paper/CPTIVIDT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1607.03147&json=true","fetch_graph":"https://pith.science/api/pith-number/CPTIVIDT53XD4S3BT56KF7DGLP/graph.json","fetch_events":"https://pith.science/api/pith-number/CPTIVIDT53XD4S3BT56KF7DGLP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CPTIVIDT53XD4S3BT56KF7DGLP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CPTIVIDT53XD4S3BT56KF7DGLP/action/storage_attestation","attest_author":"https://pith.science/pith/CPTIVIDT53XD4S3BT56KF7DGLP/action/author_attestation","sign_citation":"https://pith.science/pith/CPTIVIDT53XD4S3BT56KF7DGLP/action/citation_signature","submit_replication":"https://pith.science/pith/CPTIVIDT53XD4S3BT56KF7DGLP/action/replication_record"}},"created_at":"2026-05-18T00:59:24.431164+00:00","updated_at":"2026-05-18T00:59:24.431164+00:00"}