{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:JMMZ2VGGS2KS6SGQ67ZWJDAGDH","short_pith_number":"pith:JMMZ2VGG","schema_version":"1.0","canonical_sha256":"4b199d54c696952f48d0f7f3648c0619d0118377ee48d040cf40d6e2d69b3f2a","source":{"kind":"arxiv","id":"1506.03901","version":1},"attestation_state":"computed","paper":{"title":"The BOSS-WiggleZ overlap region II: dependence of cosmic growth on galaxy type","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Chris Blake, Donald P. Schneider, Eyal Kazin, Felipe A. Mar\\'in, Florian Beutler, Jun Koda","submitted_at":"2015-06-12T05:55:03Z","abstract_excerpt":"The anisotropic galaxy 2-point correlation function (2PCF) allows measurement of the growth of large-scale structures from the effect of peculiar velocities on the clustering pattern. We present new measurements of the auto- and cross- correlation function multipoles of 69,180 WiggleZ and 46,380 BOSS-CMASS galaxies sharing an overlapping volume of ~0.2 (Gpc/h)^3. Analysing the redshift-space distortions (RSD) of galaxy 2-point statistics for these two galaxy tracers, we test for systematic errors in the modelling depending on galaxy type and investigate potential improvements in cosmological c"},"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":"1506.03901","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2015-06-12T05:55:03Z","cross_cats_sorted":[],"title_canon_sha256":"c009b51735735307276e37da73c25dd344add459482f2a7ed3c13c1a449bdfa3","abstract_canon_sha256":"b796a172d9f978ad22711aee668f46b320185b6c21c1ba1f0cb63d9c0b19a413"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:24:54.653295Z","signature_b64":"siBX0yg/Lvp7gFBfIW7bE3yMjVWdLxkm81kCBP4hNhQOM7oPunF7EnWmPKsCw4aDN0qLMILoIoBDjdTPX9bIBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4b199d54c696952f48d0f7f3648c0619d0118377ee48d040cf40d6e2d69b3f2a","last_reissued_at":"2026-05-18T01:24:54.652722Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:24:54.652722Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The BOSS-WiggleZ overlap region II: dependence of cosmic growth on galaxy type","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Chris Blake, Donald P. Schneider, Eyal Kazin, Felipe A. Mar\\'in, Florian Beutler, Jun Koda","submitted_at":"2015-06-12T05:55:03Z","abstract_excerpt":"The anisotropic galaxy 2-point correlation function (2PCF) allows measurement of the growth of large-scale structures from the effect of peculiar velocities on the clustering pattern. We present new measurements of the auto- and cross- correlation function multipoles of 69,180 WiggleZ and 46,380 BOSS-CMASS galaxies sharing an overlapping volume of ~0.2 (Gpc/h)^3. Analysing the redshift-space distortions (RSD) of galaxy 2-point statistics for these two galaxy tracers, we test for systematic errors in the modelling depending on galaxy type and investigate potential improvements in cosmological c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.03901","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":"1506.03901","created_at":"2026-05-18T01:24:54.652833+00:00"},{"alias_kind":"arxiv_version","alias_value":"1506.03901v1","created_at":"2026-05-18T01:24:54.652833+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.03901","created_at":"2026-05-18T01:24:54.652833+00:00"},{"alias_kind":"pith_short_12","alias_value":"JMMZ2VGGS2KS","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_16","alias_value":"JMMZ2VGGS2KS6SGQ","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_8","alias_value":"JMMZ2VGG","created_at":"2026-05-18T12:29:27.538025+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JMMZ2VGGS2KS6SGQ67ZWJDAGDH","json":"https://pith.science/pith/JMMZ2VGGS2KS6SGQ67ZWJDAGDH.json","graph_json":"https://pith.science/api/pith-number/JMMZ2VGGS2KS6SGQ67ZWJDAGDH/graph.json","events_json":"https://pith.science/api/pith-number/JMMZ2VGGS2KS6SGQ67ZWJDAGDH/events.json","paper":"https://pith.science/paper/JMMZ2VGG"},"agent_actions":{"view_html":"https://pith.science/pith/JMMZ2VGGS2KS6SGQ67ZWJDAGDH","download_json":"https://pith.science/pith/JMMZ2VGGS2KS6SGQ67ZWJDAGDH.json","view_paper":"https://pith.science/paper/JMMZ2VGG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1506.03901&json=true","fetch_graph":"https://pith.science/api/pith-number/JMMZ2VGGS2KS6SGQ67ZWJDAGDH/graph.json","fetch_events":"https://pith.science/api/pith-number/JMMZ2VGGS2KS6SGQ67ZWJDAGDH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JMMZ2VGGS2KS6SGQ67ZWJDAGDH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JMMZ2VGGS2KS6SGQ67ZWJDAGDH/action/storage_attestation","attest_author":"https://pith.science/pith/JMMZ2VGGS2KS6SGQ67ZWJDAGDH/action/author_attestation","sign_citation":"https://pith.science/pith/JMMZ2VGGS2KS6SGQ67ZWJDAGDH/action/citation_signature","submit_replication":"https://pith.science/pith/JMMZ2VGGS2KS6SGQ67ZWJDAGDH/action/replication_record"}},"created_at":"2026-05-18T01:24:54.652833+00:00","updated_at":"2026-05-18T01:24:54.652833+00:00"}