{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:OIJPE2KRE7RU4K3JK2TCKN7W73","short_pith_number":"pith:OIJPE2KR","schema_version":"1.0","canonical_sha256":"7212f2695127e34e2b6956a62537f6fed2291af4eb694f9593361de6472ea6b8","source":{"kind":"arxiv","id":"1009.4190","version":1},"attestation_state":"computed","paper":{"title":"The effect of the Solar motion on the flux of long-period comets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.EP","authors_text":"C. Flynn, E. Gardner, P. Nurmi, S. Mikkola","submitted_at":"2010-09-21T20:00:01Z","abstract_excerpt":"The long-term dynamics of Oort cloud comets are studied under the influence of both the radial and the vertical components of the Galactic tidal field. Sporadic dynamical perturbation processes are ignored, such as passing stars, since we aim to study the influence of just the axisymmetric Galactic tidal field on the cometary motion and how it changes in time. We use a model of the Galaxy with a disc, bulge and dark halo, and a local disc density, and disc scale length constrained to fit the best available observational constraints. By integrating a few million of cometary orbits over 1 Gyr, w"},"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":"1009.4190","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2010-09-21T20:00:01Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"515a989dd67ff864f37df154b4449c05a7f7e740c417d1f0279c0aa86d9f72b8","abstract_canon_sha256":"43f5ae757859163de2cfec7081233826a9624a25807adf4c7dc2d2720107e323"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:33:26.772402Z","signature_b64":"0lhHjFkufoqVr3qVWT4sXEcRfrdJ/W+0ZqnuR3p5l0kAZqOj83TCwt5gDj8fsXFwLfSLk2Wl36iXt9ryuMjmCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7212f2695127e34e2b6956a62537f6fed2291af4eb694f9593361de6472ea6b8","last_reissued_at":"2026-05-18T04:33:26.771934Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:33:26.771934Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The effect of the Solar motion on the flux of long-period comets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.EP","authors_text":"C. Flynn, E. Gardner, P. Nurmi, S. Mikkola","submitted_at":"2010-09-21T20:00:01Z","abstract_excerpt":"The long-term dynamics of Oort cloud comets are studied under the influence of both the radial and the vertical components of the Galactic tidal field. Sporadic dynamical perturbation processes are ignored, such as passing stars, since we aim to study the influence of just the axisymmetric Galactic tidal field on the cometary motion and how it changes in time. We use a model of the Galaxy with a disc, bulge and dark halo, and a local disc density, and disc scale length constrained to fit the best available observational constraints. By integrating a few million of cometary orbits over 1 Gyr, w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.4190","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":"1009.4190","created_at":"2026-05-18T04:33:26.771996+00:00"},{"alias_kind":"arxiv_version","alias_value":"1009.4190v1","created_at":"2026-05-18T04:33:26.771996+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.4190","created_at":"2026-05-18T04:33:26.771996+00:00"},{"alias_kind":"pith_short_12","alias_value":"OIJPE2KRE7RU","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_16","alias_value":"OIJPE2KRE7RU4K3J","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_8","alias_value":"OIJPE2KR","created_at":"2026-05-18T12:26:12.377268+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/OIJPE2KRE7RU4K3JK2TCKN7W73","json":"https://pith.science/pith/OIJPE2KRE7RU4K3JK2TCKN7W73.json","graph_json":"https://pith.science/api/pith-number/OIJPE2KRE7RU4K3JK2TCKN7W73/graph.json","events_json":"https://pith.science/api/pith-number/OIJPE2KRE7RU4K3JK2TCKN7W73/events.json","paper":"https://pith.science/paper/OIJPE2KR"},"agent_actions":{"view_html":"https://pith.science/pith/OIJPE2KRE7RU4K3JK2TCKN7W73","download_json":"https://pith.science/pith/OIJPE2KRE7RU4K3JK2TCKN7W73.json","view_paper":"https://pith.science/paper/OIJPE2KR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1009.4190&json=true","fetch_graph":"https://pith.science/api/pith-number/OIJPE2KRE7RU4K3JK2TCKN7W73/graph.json","fetch_events":"https://pith.science/api/pith-number/OIJPE2KRE7RU4K3JK2TCKN7W73/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OIJPE2KRE7RU4K3JK2TCKN7W73/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OIJPE2KRE7RU4K3JK2TCKN7W73/action/storage_attestation","attest_author":"https://pith.science/pith/OIJPE2KRE7RU4K3JK2TCKN7W73/action/author_attestation","sign_citation":"https://pith.science/pith/OIJPE2KRE7RU4K3JK2TCKN7W73/action/citation_signature","submit_replication":"https://pith.science/pith/OIJPE2KRE7RU4K3JK2TCKN7W73/action/replication_record"}},"created_at":"2026-05-18T04:33:26.771996+00:00","updated_at":"2026-05-18T04:33:26.771996+00:00"}