{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:IUFWV7LWQPQITU4BA5FNYA7H4W","short_pith_number":"pith:IUFWV7LW","schema_version":"1.0","canonical_sha256":"450b6afd7683e089d381074adc03e7e59d235c353572c62ad8808588cb9d4e7c","source":{"kind":"arxiv","id":"1004.0696","version":2},"attestation_state":"computed","paper":{"title":"Dusty Disks around White Dwarfs I: Origin of Debris Disks","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"D. N.C. Lin, Ruobing Dong, X.-W. Liu, Yan Wang","submitted_at":"2010-04-05T20:00:07Z","abstract_excerpt":"A significant fraction of the mature FGK stars have cool dusty disks at least an orders of magnitudes brighter than the solar system's outer zodiacal light. Since such dusts must be continually replenished, they are generally assumed to be the collisional fragments of residual planetesimals analogous to the Kuiper Belt objects. At least 10% of solar type stars also bear gas giant planets. The fraction of stars with known gas giants or detectable debris disks (or both) appears to increase with the stellar mass. Here, we examine the dynamical evolution of systems of long-period gas giant planets"},"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":"1004.0696","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2010-04-05T20:00:07Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"df5c05695d9a694114aabba1be3fc54e60cacb673f22a6c8384e235a3a9b559e","abstract_canon_sha256":"3dd83954c668c3581703680f5b4a50a8bfc144e3c0ccca29ac057b582555913c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:08:14.328471Z","signature_b64":"/686wXMk/ncvH8syopauZnHRKINrwzRAGoxGb8BbiTRyJtXIQGvcLTvAFuCV2BQmu2RL2u8FxyLEJFBhXgWoDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"450b6afd7683e089d381074adc03e7e59d235c353572c62ad8808588cb9d4e7c","last_reissued_at":"2026-05-18T02:08:14.328011Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:08:14.328011Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dusty Disks around White Dwarfs I: Origin of Debris Disks","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"D. N.C. Lin, Ruobing Dong, X.-W. Liu, Yan Wang","submitted_at":"2010-04-05T20:00:07Z","abstract_excerpt":"A significant fraction of the mature FGK stars have cool dusty disks at least an orders of magnitudes brighter than the solar system's outer zodiacal light. Since such dusts must be continually replenished, they are generally assumed to be the collisional fragments of residual planetesimals analogous to the Kuiper Belt objects. At least 10% of solar type stars also bear gas giant planets. The fraction of stars with known gas giants or detectable debris disks (or both) appears to increase with the stellar mass. Here, we examine the dynamical evolution of systems of long-period gas giant planets"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1004.0696","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":"1004.0696","created_at":"2026-05-18T02:08:14.328075+00:00"},{"alias_kind":"arxiv_version","alias_value":"1004.0696v2","created_at":"2026-05-18T02:08:14.328075+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1004.0696","created_at":"2026-05-18T02:08:14.328075+00:00"},{"alias_kind":"pith_short_12","alias_value":"IUFWV7LWQPQI","created_at":"2026-05-18T12:26:09.077623+00:00"},{"alias_kind":"pith_short_16","alias_value":"IUFWV7LWQPQITU4B","created_at":"2026-05-18T12:26:09.077623+00:00"},{"alias_kind":"pith_short_8","alias_value":"IUFWV7LW","created_at":"2026-05-18T12:26:09.077623+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/IUFWV7LWQPQITU4BA5FNYA7H4W","json":"https://pith.science/pith/IUFWV7LWQPQITU4BA5FNYA7H4W.json","graph_json":"https://pith.science/api/pith-number/IUFWV7LWQPQITU4BA5FNYA7H4W/graph.json","events_json":"https://pith.science/api/pith-number/IUFWV7LWQPQITU4BA5FNYA7H4W/events.json","paper":"https://pith.science/paper/IUFWV7LW"},"agent_actions":{"view_html":"https://pith.science/pith/IUFWV7LWQPQITU4BA5FNYA7H4W","download_json":"https://pith.science/pith/IUFWV7LWQPQITU4BA5FNYA7H4W.json","view_paper":"https://pith.science/paper/IUFWV7LW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1004.0696&json=true","fetch_graph":"https://pith.science/api/pith-number/IUFWV7LWQPQITU4BA5FNYA7H4W/graph.json","fetch_events":"https://pith.science/api/pith-number/IUFWV7LWQPQITU4BA5FNYA7H4W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IUFWV7LWQPQITU4BA5FNYA7H4W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IUFWV7LWQPQITU4BA5FNYA7H4W/action/storage_attestation","attest_author":"https://pith.science/pith/IUFWV7LWQPQITU4BA5FNYA7H4W/action/author_attestation","sign_citation":"https://pith.science/pith/IUFWV7LWQPQITU4BA5FNYA7H4W/action/citation_signature","submit_replication":"https://pith.science/pith/IUFWV7LWQPQITU4BA5FNYA7H4W/action/replication_record"}},"created_at":"2026-05-18T02:08:14.328075+00:00","updated_at":"2026-05-18T02:08:14.328075+00:00"}