{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:46HTVUF7SRCAUXYNG7RTLMNHRP","short_pith_number":"pith:46HTVUF7","schema_version":"1.0","canonical_sha256":"e78f3ad0bf94440a5f0d37e335b1a78bf02a78fbdba5b28944d08022acd973e5","source":{"kind":"arxiv","id":"1607.03154","version":2},"attestation_state":"computed","paper":{"title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in configuration space","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Antonio J. Cuesta, Ariel G. S\\'anchez, Ashley J. Ross, Chia-Hsun Chuang, Daniel J. Eisenstein, Daniel Thomas, Fangzhou Zhu, Francisco Prada, Francisco-Shu Kitaura, Gong-Bo Zhao, Graziano Rossi, H\\'ector Gil-Mar\\'in, Jean-Paul Kneib, Jeremy Tinker, Joel R. Brownstein, Mariana Vargas-Maga\\~na, Matt Olmstead, Rita Tojeiro, Salvador Salazar-Albornoz, Sergio Rodriguez-Torres, Shirley Ho, Will J. Percival, Yuting Wang","submitted_at":"2016-07-11T20:29:51Z","abstract_excerpt":"We perform a tomographic baryon acoustic oscillations analysis using the two-point galaxy correlation function measured from the combined sample of BOSS DR12, which covers the redshift range of $0.2<z<0.75$. Splitting the sample into multiple overlapping redshift slices to extract the redshift information of galaxy clustering, we obtain a measurement of $D_A(z)/r_d$ and $H(z)r_d$ at nine effective redshifts with the full covariance matrix calibrated using MultiDark-Patchy mock catalogues. Using the reconstructed galaxy catalogues, we obtain the precision of $1.3\\%-2.2\\%$ for $D_A(z)/r_d$ and $"},"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":"1607.03154","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-07-11T20:29:51Z","cross_cats_sorted":[],"title_canon_sha256":"9673d0d7bd5b3b1133d41485a6ae1539853b11d113b50469a3d2ef6cea5faacb","abstract_canon_sha256":"8fcf3fb0df7625d12d28ed3bb73e6b343fb7109fc650eecaab704044eafac2d8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:41:41.586798Z","signature_b64":"zL2L9viKXrzgNpYjWHbE/oaGFovQxbVF6Cxei9MQkaLvSbPcB7OAVSUTf/yYrIxz4n2GkYt08/k7t7+N9VeGDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e78f3ad0bf94440a5f0d37e335b1a78bf02a78fbdba5b28944d08022acd973e5","last_reissued_at":"2026-05-18T00:41:41.586307Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:41:41.586307Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in configuration space","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Antonio J. Cuesta, Ariel G. S\\'anchez, Ashley J. Ross, Chia-Hsun Chuang, Daniel J. Eisenstein, Daniel Thomas, Fangzhou Zhu, Francisco Prada, Francisco-Shu Kitaura, Gong-Bo Zhao, Graziano Rossi, H\\'ector Gil-Mar\\'in, Jean-Paul Kneib, Jeremy Tinker, Joel R. Brownstein, Mariana Vargas-Maga\\~na, Matt Olmstead, Rita Tojeiro, Salvador Salazar-Albornoz, Sergio Rodriguez-Torres, Shirley Ho, Will J. Percival, Yuting Wang","submitted_at":"2016-07-11T20:29:51Z","abstract_excerpt":"We perform a tomographic baryon acoustic oscillations analysis using the two-point galaxy correlation function measured from the combined sample of BOSS DR12, which covers the redshift range of $0.2<z<0.75$. Splitting the sample into multiple overlapping redshift slices to extract the redshift information of galaxy clustering, we obtain a measurement of $D_A(z)/r_d$ and $H(z)r_d$ at nine effective redshifts with the full covariance matrix calibrated using MultiDark-Patchy mock catalogues. Using the reconstructed galaxy catalogues, we obtain the precision of $1.3\\%-2.2\\%$ for $D_A(z)/r_d$ and $"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.03154","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":"1607.03154","created_at":"2026-05-18T00:41:41.586390+00:00"},{"alias_kind":"arxiv_version","alias_value":"1607.03154v2","created_at":"2026-05-18T00:41:41.586390+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.03154","created_at":"2026-05-18T00:41:41.586390+00:00"},{"alias_kind":"pith_short_12","alias_value":"46HTVUF7SRCA","created_at":"2026-05-18T12:29:58.707656+00:00"},{"alias_kind":"pith_short_16","alias_value":"46HTVUF7SRCAUXYN","created_at":"2026-05-18T12:29:58.707656+00:00"},{"alias_kind":"pith_short_8","alias_value":"46HTVUF7","created_at":"2026-05-18T12:29:58.707656+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.01070","citing_title":"Barrow holographic dark energy interacting model in the presence of radiation and matter","ref_index":110,"is_internal_anchor":true},{"citing_arxiv_id":"2604.23793","citing_title":"From Big Bang Nucleosynthesis to Late-Time Acceleration in $f(Q,L_m)$ Gravity","ref_index":71,"is_internal_anchor":false},{"citing_arxiv_id":"2604.22450","citing_title":"Exploring Cosmic Evolution in R\\'enyi Entropic Cosmology with Constraints from DESI DR2 BAO and GW Data","ref_index":53,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/46HTVUF7SRCAUXYNG7RTLMNHRP","json":"https://pith.science/pith/46HTVUF7SRCAUXYNG7RTLMNHRP.json","graph_json":"https://pith.science/api/pith-number/46HTVUF7SRCAUXYNG7RTLMNHRP/graph.json","events_json":"https://pith.science/api/pith-number/46HTVUF7SRCAUXYNG7RTLMNHRP/events.json","paper":"https://pith.science/paper/46HTVUF7"},"agent_actions":{"view_html":"https://pith.science/pith/46HTVUF7SRCAUXYNG7RTLMNHRP","download_json":"https://pith.science/pith/46HTVUF7SRCAUXYNG7RTLMNHRP.json","view_paper":"https://pith.science/paper/46HTVUF7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1607.03154&json=true","fetch_graph":"https://pith.science/api/pith-number/46HTVUF7SRCAUXYNG7RTLMNHRP/graph.json","fetch_events":"https://pith.science/api/pith-number/46HTVUF7SRCAUXYNG7RTLMNHRP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/46HTVUF7SRCAUXYNG7RTLMNHRP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/46HTVUF7SRCAUXYNG7RTLMNHRP/action/storage_attestation","attest_author":"https://pith.science/pith/46HTVUF7SRCAUXYNG7RTLMNHRP/action/author_attestation","sign_citation":"https://pith.science/pith/46HTVUF7SRCAUXYNG7RTLMNHRP/action/citation_signature","submit_replication":"https://pith.science/pith/46HTVUF7SRCAUXYNG7RTLMNHRP/action/replication_record"}},"created_at":"2026-05-18T00:41:41.586390+00:00","updated_at":"2026-05-18T00:41:41.586390+00:00"}