{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:GGACNXJFSZX7EHHTCTVVYLX6X5","short_pith_number":"pith:GGACNXJF","schema_version":"1.0","canonical_sha256":"318026dd25966ff21cf314eb5c2efebf7bf3f0e8a8f1a640e30fbbcaa4f7fc28","source":{"kind":"arxiv","id":"1801.03062","version":1},"attestation_state":"computed","paper":{"title":"The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adam D. Myers, Ariel G. Sanchez, Ashley J. Ross, Cheng Zhao, Chia-Hsun Chuang, Christophe Y\\`eche, Donald P. Schneider, Etienne Burtin, Falk Baumgarten, Francisco Prada, Gong-Bo Zhao, Graziano Rossi, Hector Gil-Marin, Hee-Jong Seo, H\\'elion du Mas des Bourboux, Isabelle Paris, Jean-Marc Le Goff, Jean-Paul Kneib, Jeremy L. Tinker, Jiamin Hou, Joel R. Brownstein, Johan Comparat, John Peacock, Julian Bautista, Katrin Heitmann, Kyle S. Dawson, Nathalie Palanque-Delabrouille, Patrick Petitjean, Pauline Zarrouk, Pierre Laurent, Rita Tojeiro, Rossana Ruggeri, Salman Habib, Sergio A. Rodriguez-Torres, Sylvain de la Torre, Violeta Gonzalez-Perez, Will J. Percival, Yuting Wang","submitted_at":"2018-01-09T17:54:06Z","abstract_excerpt":"We present the clustering measurements of quasars in configuration space based on the Data Release 14 (DR14) of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey. This dataset includes 148,659 quasars spread over the redshift range $0.8\\leq z \\leq 2.2$ and spanning 2112.9 square degrees. We use the Convolution Lagrangian Perturbation Theory (CLPT) approach with a Gaussian Streaming (GS) model for the redshift space distortions of the correlation function and demonstrate its applicability for dark matter halos hosting eBOSS quasar tracers. At the effective redshif"},"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":"1801.03062","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2018-01-09T17:54:06Z","cross_cats_sorted":[],"title_canon_sha256":"a9c791d635e6cefa7577e9cb9bc1be031b194f309430f7a0ca9ca50bcb0c7c61","abstract_canon_sha256":"4bff2054b0b06b1e6f7c2980db1e22e2cd07822d105bf09ca6bdf420f0ae92a2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:22:02.367441Z","signature_b64":"L5R7cUWRNBaLLWKU2uAGeFzjY/RBDJLrBvhqw7LGG4ekhlSCnr3/1pXq3q3F0MfHBRGi3QUrzq/+ufWV7eXWAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"318026dd25966ff21cf314eb5c2efebf7bf3f0e8a8f1a640e30fbbcaa4f7fc28","last_reissued_at":"2026-05-18T00:22:02.366941Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:22:02.366941Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adam D. Myers, Ariel G. Sanchez, Ashley J. Ross, Cheng Zhao, Chia-Hsun Chuang, Christophe Y\\`eche, Donald P. Schneider, Etienne Burtin, Falk Baumgarten, Francisco Prada, Gong-Bo Zhao, Graziano Rossi, Hector Gil-Marin, Hee-Jong Seo, H\\'elion du Mas des Bourboux, Isabelle Paris, Jean-Marc Le Goff, Jean-Paul Kneib, Jeremy L. Tinker, Jiamin Hou, Joel R. Brownstein, Johan Comparat, John Peacock, Julian Bautista, Katrin Heitmann, Kyle S. Dawson, Nathalie Palanque-Delabrouille, Patrick Petitjean, Pauline Zarrouk, Pierre Laurent, Rita Tojeiro, Rossana Ruggeri, Salman Habib, Sergio A. Rodriguez-Torres, Sylvain de la Torre, Violeta Gonzalez-Perez, Will J. Percival, Yuting Wang","submitted_at":"2018-01-09T17:54:06Z","abstract_excerpt":"We present the clustering measurements of quasars in configuration space based on the Data Release 14 (DR14) of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey. This dataset includes 148,659 quasars spread over the redshift range $0.8\\leq z \\leq 2.2$ and spanning 2112.9 square degrees. We use the Convolution Lagrangian Perturbation Theory (CLPT) approach with a Gaussian Streaming (GS) model for the redshift space distortions of the correlation function and demonstrate its applicability for dark matter halos hosting eBOSS quasar tracers. At the effective redshif"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.03062","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":"1801.03062","created_at":"2026-05-18T00:22:02.367017+00:00"},{"alias_kind":"arxiv_version","alias_value":"1801.03062v1","created_at":"2026-05-18T00:22:02.367017+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1801.03062","created_at":"2026-05-18T00:22:02.367017+00:00"},{"alias_kind":"pith_short_12","alias_value":"GGACNXJFSZX7","created_at":"2026-05-18T12:32:25.280505+00:00"},{"alias_kind":"pith_short_16","alias_value":"GGACNXJFSZX7EHHT","created_at":"2026-05-18T12:32:25.280505+00:00"},{"alias_kind":"pith_short_8","alias_value":"GGACNXJF","created_at":"2026-05-18T12:32:25.280505+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.18723","citing_title":"Model-independent reconstruction of cosmic thermodynamics and dark energy dynamics","ref_index":13,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GGACNXJFSZX7EHHTCTVVYLX6X5","json":"https://pith.science/pith/GGACNXJFSZX7EHHTCTVVYLX6X5.json","graph_json":"https://pith.science/api/pith-number/GGACNXJFSZX7EHHTCTVVYLX6X5/graph.json","events_json":"https://pith.science/api/pith-number/GGACNXJFSZX7EHHTCTVVYLX6X5/events.json","paper":"https://pith.science/paper/GGACNXJF"},"agent_actions":{"view_html":"https://pith.science/pith/GGACNXJFSZX7EHHTCTVVYLX6X5","download_json":"https://pith.science/pith/GGACNXJFSZX7EHHTCTVVYLX6X5.json","view_paper":"https://pith.science/paper/GGACNXJF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1801.03062&json=true","fetch_graph":"https://pith.science/api/pith-number/GGACNXJFSZX7EHHTCTVVYLX6X5/graph.json","fetch_events":"https://pith.science/api/pith-number/GGACNXJFSZX7EHHTCTVVYLX6X5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GGACNXJFSZX7EHHTCTVVYLX6X5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GGACNXJFSZX7EHHTCTVVYLX6X5/action/storage_attestation","attest_author":"https://pith.science/pith/GGACNXJFSZX7EHHTCTVVYLX6X5/action/author_attestation","sign_citation":"https://pith.science/pith/GGACNXJFSZX7EHHTCTVVYLX6X5/action/citation_signature","submit_replication":"https://pith.science/pith/GGACNXJFSZX7EHHTCTVVYLX6X5/action/replication_record"}},"created_at":"2026-05-18T00:22:02.367017+00:00","updated_at":"2026-05-18T00:22:02.367017+00:00"}