{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:I4R6FPUUW56WPMYOAIAQ2UFX7Q","short_pith_number":"pith:I4R6FPUU","schema_version":"1.0","canonical_sha256":"4723e2be94b77d67b30e02010d50b7fc05e46f686ff81e246468cbcfa3b3bde4","source":{"kind":"arxiv","id":"0911.5347","version":4},"attestation_state":"computed","paper":{"title":"The WiggleZ Dark Energy Survey: Direct constraints on blue galaxy intrinsic alignments at intermediate redshifts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Barry Madore, Ben Jelliffe, Chris Blake, Chris Martin, David Woods, Emily Wisnioski, Filipe B. Abdalla, Gregory B. Poole, I-hui Li, Karl Forster, Karl Glazebrook, Kevin Pimbblet, Matthew Colless, Michael J. Drinkwater, Michael Pracy, Rachel Mandelbaum, Rob Sharp, Russell J. Jurek, Sarah Bridle, Sarah Brough, Scott Croom, Tamara Davis, Ted Wyder, Warrick Couch","submitted_at":"2009-11-27T21:04:52Z","abstract_excerpt":"Correlations between the intrinsic shapes of galaxy pairs, and between the intrinsic shapes of galaxies and the large-scale density field, may be induced by tidal fields. These correlations, which have been detected at low redshifts (z<0.35) for bright red galaxies in the Sloan Digital Sky Survey (SDSS), and for which upper limits exist for blue galaxies at z~0.1, provide a window into galaxy formation and evolution, and are also an important contaminant for current and future weak lensing surveys. Measurements of these alignments at intermediate redshifts (z~0.6) that are more relevant for co"},"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":"0911.5347","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2009-11-27T21:04:52Z","cross_cats_sorted":[],"title_canon_sha256":"5f24de6248bdc973e1641146382806641dc5466d3c491d6a1a855adef55beff6","abstract_canon_sha256":"3d9809172959721f6ad111b997ebead3603c675dc52c47a442b88036b71ac4b4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:10:36.037872Z","signature_b64":"+F2g4U16YnljrJt7HPL6QlX5AKP3rTvLNNKPoD8p3bjLgOPDTpkiWSXyFnIELPlrTLs3wWuPhkz0GyNvy4oLCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4723e2be94b77d67b30e02010d50b7fc05e46f686ff81e246468cbcfa3b3bde4","last_reissued_at":"2026-05-18T02:10:36.036985Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:10:36.036985Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The WiggleZ Dark Energy Survey: Direct constraints on blue galaxy intrinsic alignments at intermediate redshifts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Barry Madore, Ben Jelliffe, Chris Blake, Chris Martin, David Woods, Emily Wisnioski, Filipe B. Abdalla, Gregory B. Poole, I-hui Li, Karl Forster, Karl Glazebrook, Kevin Pimbblet, Matthew Colless, Michael J. Drinkwater, Michael Pracy, Rachel Mandelbaum, Rob Sharp, Russell J. Jurek, Sarah Bridle, Sarah Brough, Scott Croom, Tamara Davis, Ted Wyder, Warrick Couch","submitted_at":"2009-11-27T21:04:52Z","abstract_excerpt":"Correlations between the intrinsic shapes of galaxy pairs, and between the intrinsic shapes of galaxies and the large-scale density field, may be induced by tidal fields. These correlations, which have been detected at low redshifts (z<0.35) for bright red galaxies in the Sloan Digital Sky Survey (SDSS), and for which upper limits exist for blue galaxies at z~0.1, provide a window into galaxy formation and evolution, and are also an important contaminant for current and future weak lensing surveys. Measurements of these alignments at intermediate redshifts (z~0.6) that are more relevant for co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0911.5347","kind":"arxiv","version":4},"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":"0911.5347","created_at":"2026-05-18T02:10:36.037106+00:00"},{"alias_kind":"arxiv_version","alias_value":"0911.5347v4","created_at":"2026-05-18T02:10:36.037106+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0911.5347","created_at":"2026-05-18T02:10:36.037106+00:00"},{"alias_kind":"pith_short_12","alias_value":"I4R6FPUUW56W","created_at":"2026-05-18T12:25:59.703012+00:00"},{"alias_kind":"pith_short_16","alias_value":"I4R6FPUUW56WPMYO","created_at":"2026-05-18T12:25:59.703012+00:00"},{"alias_kind":"pith_short_8","alias_value":"I4R6FPUU","created_at":"2026-05-18T12:25:59.703012+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.11658","citing_title":"GI BAO as a cosmological consistency check","ref_index":47,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/I4R6FPUUW56WPMYOAIAQ2UFX7Q","json":"https://pith.science/pith/I4R6FPUUW56WPMYOAIAQ2UFX7Q.json","graph_json":"https://pith.science/api/pith-number/I4R6FPUUW56WPMYOAIAQ2UFX7Q/graph.json","events_json":"https://pith.science/api/pith-number/I4R6FPUUW56WPMYOAIAQ2UFX7Q/events.json","paper":"https://pith.science/paper/I4R6FPUU"},"agent_actions":{"view_html":"https://pith.science/pith/I4R6FPUUW56WPMYOAIAQ2UFX7Q","download_json":"https://pith.science/pith/I4R6FPUUW56WPMYOAIAQ2UFX7Q.json","view_paper":"https://pith.science/paper/I4R6FPUU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0911.5347&json=true","fetch_graph":"https://pith.science/api/pith-number/I4R6FPUUW56WPMYOAIAQ2UFX7Q/graph.json","fetch_events":"https://pith.science/api/pith-number/I4R6FPUUW56WPMYOAIAQ2UFX7Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I4R6FPUUW56WPMYOAIAQ2UFX7Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I4R6FPUUW56WPMYOAIAQ2UFX7Q/action/storage_attestation","attest_author":"https://pith.science/pith/I4R6FPUUW56WPMYOAIAQ2UFX7Q/action/author_attestation","sign_citation":"https://pith.science/pith/I4R6FPUUW56WPMYOAIAQ2UFX7Q/action/citation_signature","submit_replication":"https://pith.science/pith/I4R6FPUUW56WPMYOAIAQ2UFX7Q/action/replication_record"}},"created_at":"2026-05-18T02:10:36.037106+00:00","updated_at":"2026-05-18T02:10:36.037106+00:00"}