{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:5T4ZV4BFNOFNQWSADEPWK2PNOW","short_pith_number":"pith:5T4ZV4BF","schema_version":"1.0","canonical_sha256":"ecf99af0256b8ad85a40191f6569ed75b231e042cf8b413271ac1754ba9eaf70","source":{"kind":"arxiv","id":"1603.05184","version":2},"attestation_state":"computed","paper":{"title":"Redshift-space distortions around voids","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Andy Taylor (IfA, Edinburgh), John A. Peacock (IfA, Nelson Padilla (Cat\\'olica), Yan-Chuan Cai (IfA","submitted_at":"2016-03-16T17:26:06Z","abstract_excerpt":"We have derived estimators for the linear growth rate of density fluctuations using the cross-correlation function of voids and haloes in redshift space, both directly and in Fourier form. In linear theory, this cross-correlation contains only monopole and quadrupole terms. At scales greater than the void radius, linear theory is a good match to voids traced out by haloes in N-body simulations; small-scale random velocities are unimportant at these radii, only tending to cause small and often negligible elongation of the redshift-space cross-correlation function near its origin. By extracting "},"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":"1603.05184","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-03-16T17:26:06Z","cross_cats_sorted":[],"title_canon_sha256":"d9974835310521bb61de23395e083c79050773b49357d463c2970160843e3ae9","abstract_canon_sha256":"47fd7b154fcd76da5c4715cfc360947281f6b04c801873b020eac9aa080baddf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:09:35.961470Z","signature_b64":"0TDT7mgcYIMYXrU5tNZJ7sLIR51IovwrFLkRZVMNGFE857Hga+zFRE17UOQI4V7obVZw8zKooRPLEIQ55U+OBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ecf99af0256b8ad85a40191f6569ed75b231e042cf8b413271ac1754ba9eaf70","last_reissued_at":"2026-05-18T01:09:35.960995Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:09:35.960995Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Redshift-space distortions around voids","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Andy Taylor (IfA, Edinburgh), John A. Peacock (IfA, Nelson Padilla (Cat\\'olica), Yan-Chuan Cai (IfA","submitted_at":"2016-03-16T17:26:06Z","abstract_excerpt":"We have derived estimators for the linear growth rate of density fluctuations using the cross-correlation function of voids and haloes in redshift space, both directly and in Fourier form. In linear theory, this cross-correlation contains only monopole and quadrupole terms. At scales greater than the void radius, linear theory is a good match to voids traced out by haloes in N-body simulations; small-scale random velocities are unimportant at these radii, only tending to cause small and often negligible elongation of the redshift-space cross-correlation function near its origin. By extracting "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.05184","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":"1603.05184","created_at":"2026-05-18T01:09:35.961070+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.05184v2","created_at":"2026-05-18T01:09:35.961070+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.05184","created_at":"2026-05-18T01:09:35.961070+00:00"},{"alias_kind":"pith_short_12","alias_value":"5T4ZV4BFNOFN","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_16","alias_value":"5T4ZV4BFNOFNQWSA","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_8","alias_value":"5T4ZV4BF","created_at":"2026-05-18T12:30:01.593930+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.12482","citing_title":"Unveiling $f(R)$ Gravity with Void-Galaxy Cross-Correlation Multipoles","ref_index":70,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5T4ZV4BFNOFNQWSADEPWK2PNOW","json":"https://pith.science/pith/5T4ZV4BFNOFNQWSADEPWK2PNOW.json","graph_json":"https://pith.science/api/pith-number/5T4ZV4BFNOFNQWSADEPWK2PNOW/graph.json","events_json":"https://pith.science/api/pith-number/5T4ZV4BFNOFNQWSADEPWK2PNOW/events.json","paper":"https://pith.science/paper/5T4ZV4BF"},"agent_actions":{"view_html":"https://pith.science/pith/5T4ZV4BFNOFNQWSADEPWK2PNOW","download_json":"https://pith.science/pith/5T4ZV4BFNOFNQWSADEPWK2PNOW.json","view_paper":"https://pith.science/paper/5T4ZV4BF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.05184&json=true","fetch_graph":"https://pith.science/api/pith-number/5T4ZV4BFNOFNQWSADEPWK2PNOW/graph.json","fetch_events":"https://pith.science/api/pith-number/5T4ZV4BFNOFNQWSADEPWK2PNOW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5T4ZV4BFNOFNQWSADEPWK2PNOW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5T4ZV4BFNOFNQWSADEPWK2PNOW/action/storage_attestation","attest_author":"https://pith.science/pith/5T4ZV4BFNOFNQWSADEPWK2PNOW/action/author_attestation","sign_citation":"https://pith.science/pith/5T4ZV4BFNOFNQWSADEPWK2PNOW/action/citation_signature","submit_replication":"https://pith.science/pith/5T4ZV4BFNOFNQWSADEPWK2PNOW/action/replication_record"}},"created_at":"2026-05-18T01:09:35.961070+00:00","updated_at":"2026-05-18T01:09:35.961070+00:00"}