{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:GX4ZYYPT3PUZCTPXTDJ55MUY5G","short_pith_number":"pith:GX4ZYYPT","schema_version":"1.0","canonical_sha256":"35f99c61f3dbe9914df798d3deb298e99d7e4274694129626371bc30dcbd4862","source":{"kind":"arxiv","id":"2401.06002","version":2},"attestation_state":"computed","paper":{"title":"A 3D Diffusive and Advective Model of Electron Transport Applied to the Pulsar Wind Nebula HESS J1825-137","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Fabien Voisin, Gavin Rowell, Hidetoshi Sano, Sabrina Einecke, Tiffany Collins, Yasuo Fukui","submitted_at":"2024-01-11T16:05:43Z","abstract_excerpt":"HESS J1825-137 is one of the most powerful and luminous TeV gamma-ray pulsar wind nebulae (PWNe), making it an excellent laboratory to study particle transportation around pulsars. We present a model of the (diffusive and advective) transport and radiative losses of electrons from the pulsar PSRJ1826-1334 powering HESSJ1825-137 using interstellar medium gas (ISM) data, soft photon fields and a spatially varying magnetic field. We find that for the characteristic age of 21 kyr, PSR J1826-1334 is unable to meet the energy requirements to match the observed X-ray and gamma-ray emission. An older "},"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":"2401.06002","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-01-11T16:05:43Z","cross_cats_sorted":[],"title_canon_sha256":"11fc329ce4a1fee2a0684600d104a3b64b38f1dbef18876c94b695f3a6ebf971","abstract_canon_sha256":"e0c50c1e1e8817ab91dc7e91d444ac741414360f829bf5f041aaf7606e8e1f15"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:04:36.974888Z","signature_b64":"K5w87EkLrVsMynnWzJaHiD5C8bZcBM+NSMlTjEUYR5uLzg7ozfeOKQWHCICsRYisUs/8qxSQrSkrzCSyeqMdAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"35f99c61f3dbe9914df798d3deb298e99d7e4274694129626371bc30dcbd4862","last_reissued_at":"2026-07-05T08:04:36.974407Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:04:36.974407Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A 3D Diffusive and Advective Model of Electron Transport Applied to the Pulsar Wind Nebula HESS J1825-137","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Fabien Voisin, Gavin Rowell, Hidetoshi Sano, Sabrina Einecke, Tiffany Collins, Yasuo Fukui","submitted_at":"2024-01-11T16:05:43Z","abstract_excerpt":"HESS J1825-137 is one of the most powerful and luminous TeV gamma-ray pulsar wind nebulae (PWNe), making it an excellent laboratory to study particle transportation around pulsars. We present a model of the (diffusive and advective) transport and radiative losses of electrons from the pulsar PSRJ1826-1334 powering HESSJ1825-137 using interstellar medium gas (ISM) data, soft photon fields and a spatially varying magnetic field. We find that for the characteristic age of 21 kyr, PSR J1826-1334 is unable to meet the energy requirements to match the observed X-ray and gamma-ray emission. An older "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2401.06002","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2401.06002/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":"2401.06002","created_at":"2026-07-05T08:04:36.974469+00:00"},{"alias_kind":"arxiv_version","alias_value":"2401.06002v2","created_at":"2026-07-05T08:04:36.974469+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2401.06002","created_at":"2026-07-05T08:04:36.974469+00:00"},{"alias_kind":"pith_short_12","alias_value":"GX4ZYYPT3PUZ","created_at":"2026-07-05T08:04:36.974469+00:00"},{"alias_kind":"pith_short_16","alias_value":"GX4ZYYPT3PUZCTPX","created_at":"2026-07-05T08:04:36.974469+00:00"},{"alias_kind":"pith_short_8","alias_value":"GX4ZYYPT","created_at":"2026-07-05T08:04:36.974469+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/GX4ZYYPT3PUZCTPXTDJ55MUY5G","json":"https://pith.science/pith/GX4ZYYPT3PUZCTPXTDJ55MUY5G.json","graph_json":"https://pith.science/api/pith-number/GX4ZYYPT3PUZCTPXTDJ55MUY5G/graph.json","events_json":"https://pith.science/api/pith-number/GX4ZYYPT3PUZCTPXTDJ55MUY5G/events.json","paper":"https://pith.science/paper/GX4ZYYPT"},"agent_actions":{"view_html":"https://pith.science/pith/GX4ZYYPT3PUZCTPXTDJ55MUY5G","download_json":"https://pith.science/pith/GX4ZYYPT3PUZCTPXTDJ55MUY5G.json","view_paper":"https://pith.science/paper/GX4ZYYPT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2401.06002&json=true","fetch_graph":"https://pith.science/api/pith-number/GX4ZYYPT3PUZCTPXTDJ55MUY5G/graph.json","fetch_events":"https://pith.science/api/pith-number/GX4ZYYPT3PUZCTPXTDJ55MUY5G/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GX4ZYYPT3PUZCTPXTDJ55MUY5G/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GX4ZYYPT3PUZCTPXTDJ55MUY5G/action/storage_attestation","attest_author":"https://pith.science/pith/GX4ZYYPT3PUZCTPXTDJ55MUY5G/action/author_attestation","sign_citation":"https://pith.science/pith/GX4ZYYPT3PUZCTPXTDJ55MUY5G/action/citation_signature","submit_replication":"https://pith.science/pith/GX4ZYYPT3PUZCTPXTDJ55MUY5G/action/replication_record"}},"created_at":"2026-07-05T08:04:36.974469+00:00","updated_at":"2026-07-05T08:04:36.974469+00:00"}