{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1995:D3DKKWBTIN4FLKCJDCXO2BPUVY","short_pith_number":"pith:D3DKKWBT","schema_version":"1.0","canonical_sha256":"1ec6a55833437855a84918aeed05f4ae2a983f7899c2c532e9c425bf8b98ec8d","source":{"kind":"arxiv","id":"astro-ph/9501025","version":1},"attestation_state":"computed","paper":{"title":"INDICATIONS OF DARK MATTER DERIVED FROM LARGE SCALE FLOWS","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Adi Nusser, Marc Davis","submitted_at":"1995-01-09T06:17:51Z","abstract_excerpt":"Recent progress in the measurement of relative distances to galaxies has been quite substantial, and catalogs of 3000 galaxies with distances are soon to become available. The peculiar {\\it velocity} field (deviations from Hubble flow) derivable from these catalogs, when compared to the peculiar {\\it gravity} field derived from all sky redshift surveys of galaxies such as the 1.2Jy IRAS survey, leads to a unique and extremely powerful test of the density parameter $\\beta \\equiv \\Omega^{0.6}/b_I$, where $b_I$ is the possible linear bias of the IRAS selected galaxies relative to the mass fluctua"},"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":"astro-ph/9501025","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1995-01-09T06:17:51Z","cross_cats_sorted":[],"title_canon_sha256":"374a126bd5e0bed5e15a5514f4f3e75a062b96dd4553ae4d474c05a9f5041936","abstract_canon_sha256":"12bea8553f1861e928b59e628d1f2f2d94567e8e00f6581d26955d37eeab5084"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:07:42.792765Z","signature_b64":"fZp1I769rmwld7Fa1Pdq+CTh6IrinYdyGglOzaPODXgxA5k5z7P4OuBI6WgMFmjlyolj9j0cKnMGi+3i9+pzBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1ec6a55833437855a84918aeed05f4ae2a983f7899c2c532e9c425bf8b98ec8d","last_reissued_at":"2026-05-18T01:07:42.792311Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:07:42.792311Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"INDICATIONS OF DARK MATTER DERIVED FROM LARGE SCALE FLOWS","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Adi Nusser, Marc Davis","submitted_at":"1995-01-09T06:17:51Z","abstract_excerpt":"Recent progress in the measurement of relative distances to galaxies has been quite substantial, and catalogs of 3000 galaxies with distances are soon to become available. The peculiar {\\it velocity} field (deviations from Hubble flow) derivable from these catalogs, when compared to the peculiar {\\it gravity} field derived from all sky redshift surveys of galaxies such as the 1.2Jy IRAS survey, leads to a unique and extremely powerful test of the density parameter $\\beta \\equiv \\Omega^{0.6}/b_I$, where $b_I$ is the possible linear bias of the IRAS selected galaxies relative to the mass fluctua"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9501025","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":"astro-ph/9501025","created_at":"2026-05-18T01:07:42.792401+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9501025v1","created_at":"2026-05-18T01:07:42.792401+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9501025","created_at":"2026-05-18T01:07:42.792401+00:00"},{"alias_kind":"pith_short_12","alias_value":"D3DKKWBTIN4F","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_16","alias_value":"D3DKKWBTIN4FLKCJ","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_8","alias_value":"D3DKKWBT","created_at":"2026-05-18T12:25:47.700082+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/D3DKKWBTIN4FLKCJDCXO2BPUVY","json":"https://pith.science/pith/D3DKKWBTIN4FLKCJDCXO2BPUVY.json","graph_json":"https://pith.science/api/pith-number/D3DKKWBTIN4FLKCJDCXO2BPUVY/graph.json","events_json":"https://pith.science/api/pith-number/D3DKKWBTIN4FLKCJDCXO2BPUVY/events.json","paper":"https://pith.science/paper/D3DKKWBT"},"agent_actions":{"view_html":"https://pith.science/pith/D3DKKWBTIN4FLKCJDCXO2BPUVY","download_json":"https://pith.science/pith/D3DKKWBTIN4FLKCJDCXO2BPUVY.json","view_paper":"https://pith.science/paper/D3DKKWBT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9501025&json=true","fetch_graph":"https://pith.science/api/pith-number/D3DKKWBTIN4FLKCJDCXO2BPUVY/graph.json","fetch_events":"https://pith.science/api/pith-number/D3DKKWBTIN4FLKCJDCXO2BPUVY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/D3DKKWBTIN4FLKCJDCXO2BPUVY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/D3DKKWBTIN4FLKCJDCXO2BPUVY/action/storage_attestation","attest_author":"https://pith.science/pith/D3DKKWBTIN4FLKCJDCXO2BPUVY/action/author_attestation","sign_citation":"https://pith.science/pith/D3DKKWBTIN4FLKCJDCXO2BPUVY/action/citation_signature","submit_replication":"https://pith.science/pith/D3DKKWBTIN4FLKCJDCXO2BPUVY/action/replication_record"}},"created_at":"2026-05-18T01:07:42.792401+00:00","updated_at":"2026-05-18T01:07:42.792401+00:00"}