{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2000:VTJCIBFGUXWQK5OWKJNW25O7IF","short_pith_number":"pith:VTJCIBFG","schema_version":"1.0","canonical_sha256":"acd22404a6a5ed0575d6525b6d75df417a7482124fd32222c185aacea2299698","source":{"kind":"arxiv","id":"astro-ph/0002038","version":1},"attestation_state":"computed","paper":{"title":"A Search for Resonant Structures in the Zodiacal Cloud with COBE DIRBE: The Mars Wake and Jupiter's Trojan Clouds","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Marc J. Kuchner (Caltech), Michael E. Brown (Caltech), William T. Reach (IPAC/Caltech)","submitted_at":"2000-02-02T04:36:22Z","abstract_excerpt":"We searched the COBE DIRBE Sky and Zodi Atlas for a wake of dust trailing Mars and for Trojan dust near Jupiter's L5 Lagrange point. We compare the DIRBE images to a model Mars wake based on the empirical model of the Earth's wake as seen by the DIRBE and place a 3-sigma upper limit on the fractional overdensity of particles in the Mars wake of 18% of the fractional overdensity trailing the Earth. We place a 3-sigma upper limit on the effective emitting area of large (10-100 micron diameter) particles trapped at Jupiter's L5 Lagrange point of 6 x 10^17 cm^2, assuming that these large dust grai"},"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/0002038","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2000-02-02T04:36:22Z","cross_cats_sorted":[],"title_canon_sha256":"0c24ee3b8740faab892a88415ab121643ef7d7997f8879918c9a28d6d873077f","abstract_canon_sha256":"d0940ceb158d8a120d3b7004346e04b72f69ad2d93f3bbf416db48ba993922d4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:16:00.388185Z","signature_b64":"h+rK1wfG3XjnkpnipEIcOn8RGTR1lI9kxJ0EouP6lPMPIihnVziuXUC0nwD7V9WM6cbetNyfyAQ3h42Dj+L1CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"acd22404a6a5ed0575d6525b6d75df417a7482124fd32222c185aacea2299698","last_reissued_at":"2026-07-04T16:16:00.387701Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:16:00.387701Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Search for Resonant Structures in the Zodiacal Cloud with COBE DIRBE: The Mars Wake and Jupiter's Trojan Clouds","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Marc J. Kuchner (Caltech), Michael E. Brown (Caltech), William T. Reach (IPAC/Caltech)","submitted_at":"2000-02-02T04:36:22Z","abstract_excerpt":"We searched the COBE DIRBE Sky and Zodi Atlas for a wake of dust trailing Mars and for Trojan dust near Jupiter's L5 Lagrange point. We compare the DIRBE images to a model Mars wake based on the empirical model of the Earth's wake as seen by the DIRBE and place a 3-sigma upper limit on the fractional overdensity of particles in the Mars wake of 18% of the fractional overdensity trailing the Earth. We place a 3-sigma upper limit on the effective emitting area of large (10-100 micron diameter) particles trapped at Jupiter's L5 Lagrange point of 6 x 10^17 cm^2, assuming that these large dust grai"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0002038","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0002038/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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/0002038","created_at":"2026-07-04T16:16:00.387813+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0002038v1","created_at":"2026-07-04T16:16:00.387813+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0002038","created_at":"2026-07-04T16:16:00.387813+00:00"},{"alias_kind":"pith_short_12","alias_value":"VTJCIBFGUXWQ","created_at":"2026-07-04T16:16:00.387813+00:00"},{"alias_kind":"pith_short_16","alias_value":"VTJCIBFGUXWQK5OW","created_at":"2026-07-04T16:16:00.387813+00:00"},{"alias_kind":"pith_short_8","alias_value":"VTJCIBFG","created_at":"2026-07-04T16:16:00.387813+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/VTJCIBFGUXWQK5OWKJNW25O7IF","json":"https://pith.science/pith/VTJCIBFGUXWQK5OWKJNW25O7IF.json","graph_json":"https://pith.science/api/pith-number/VTJCIBFGUXWQK5OWKJNW25O7IF/graph.json","events_json":"https://pith.science/api/pith-number/VTJCIBFGUXWQK5OWKJNW25O7IF/events.json","paper":"https://pith.science/paper/VTJCIBFG"},"agent_actions":{"view_html":"https://pith.science/pith/VTJCIBFGUXWQK5OWKJNW25O7IF","download_json":"https://pith.science/pith/VTJCIBFGUXWQK5OWKJNW25O7IF.json","view_paper":"https://pith.science/paper/VTJCIBFG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0002038&json=true","fetch_graph":"https://pith.science/api/pith-number/VTJCIBFGUXWQK5OWKJNW25O7IF/graph.json","fetch_events":"https://pith.science/api/pith-number/VTJCIBFGUXWQK5OWKJNW25O7IF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VTJCIBFGUXWQK5OWKJNW25O7IF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VTJCIBFGUXWQK5OWKJNW25O7IF/action/storage_attestation","attest_author":"https://pith.science/pith/VTJCIBFGUXWQK5OWKJNW25O7IF/action/author_attestation","sign_citation":"https://pith.science/pith/VTJCIBFGUXWQK5OWKJNW25O7IF/action/citation_signature","submit_replication":"https://pith.science/pith/VTJCIBFGUXWQK5OWKJNW25O7IF/action/replication_record"}},"created_at":"2026-07-04T16:16:00.387813+00:00","updated_at":"2026-07-04T16:16:00.387813+00:00"}