{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:7TESLSNF6FRCPWL4PQWUDCACHL","short_pith_number":"pith:7TESLSNF","schema_version":"1.0","canonical_sha256":"fcc925c9a5f16227d97c7c2d4188023aeafd8c927bb440d0b008a574bd5953b6","source":{"kind":"arxiv","id":"2606.28115","version":1},"attestation_state":"computed","paper":{"title":"A Unified Model for the Emission of Supernova-Associated Fast X-ray Transients: Case Studies of EP240414a, EP250108a, and GRB~171205A","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Da-Bin Lin, En-Wei Liang, Jia Ren, Yu-Fei Li, Zhi-Lin Chen","submitted_at":"2026-06-26T14:16:56Z","abstract_excerpt":"The Einstein Probe (EP) has detected several Fast X-ray Transients (FXTs) associated with broad-lined Type Ic supernovae (SNe), including EP240414a and EP250108a. The observations reveal common features among these FXTs, but the corresponding physical origin remains debated. By comparing the FXTs with low-luminosity gamma-ray bursts (e.g., GRB 171205A), we propose a unified model that explains the common features in these events. In this model, a rapidly spinning magnetar generates a collimated Poynting flux-dominated jet and an isotropic wind. As the jet propagates through the stellar envelop"},"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":"2606.28115","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/publicdomain/zero/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-06-26T14:16:56Z","cross_cats_sorted":[],"title_canon_sha256":"61f72e4bb5b8066465a5ef68abebedb73a1fcbfe266c896ce30bb6b2ce4be51c","abstract_canon_sha256":"2ab8b168d4c9de5c04bbe281c1875ed2360159996297a2400dec5c07b4cb3ca3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-29T01:15:06.460938Z","signature_b64":"wZ9TN6paQ2Ft6WU2kqltpVYfF1be1Gcot2Dnng2llMwrs1AsdAWCy5jcDz6cwYt83ohl0NZJpjhKgb7BEPI3BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fcc925c9a5f16227d97c7c2d4188023aeafd8c927bb440d0b008a574bd5953b6","last_reissued_at":"2026-06-29T01:15:06.460517Z","signature_status":"signed_v1","first_computed_at":"2026-06-29T01:15:06.460517Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Unified Model for the Emission of Supernova-Associated Fast X-ray Transients: Case Studies of EP240414a, EP250108a, and GRB~171205A","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Da-Bin Lin, En-Wei Liang, Jia Ren, Yu-Fei Li, Zhi-Lin Chen","submitted_at":"2026-06-26T14:16:56Z","abstract_excerpt":"The Einstein Probe (EP) has detected several Fast X-ray Transients (FXTs) associated with broad-lined Type Ic supernovae (SNe), including EP240414a and EP250108a. The observations reveal common features among these FXTs, but the corresponding physical origin remains debated. By comparing the FXTs with low-luminosity gamma-ray bursts (e.g., GRB 171205A), we propose a unified model that explains the common features in these events. In this model, a rapidly spinning magnetar generates a collimated Poynting flux-dominated jet and an isotropic wind. As the jet propagates through the stellar envelop"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.28115","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/2606.28115/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":"2606.28115","created_at":"2026-06-29T01:15:06.460573+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.28115v1","created_at":"2026-06-29T01:15:06.460573+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.28115","created_at":"2026-06-29T01:15:06.460573+00:00"},{"alias_kind":"pith_short_12","alias_value":"7TESLSNF6FRC","created_at":"2026-06-29T01:15:06.460573+00:00"},{"alias_kind":"pith_short_16","alias_value":"7TESLSNF6FRCPWL4","created_at":"2026-06-29T01:15:06.460573+00:00"},{"alias_kind":"pith_short_8","alias_value":"7TESLSNF","created_at":"2026-06-29T01:15:06.460573+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/7TESLSNF6FRCPWL4PQWUDCACHL","json":"https://pith.science/pith/7TESLSNF6FRCPWL4PQWUDCACHL.json","graph_json":"https://pith.science/api/pith-number/7TESLSNF6FRCPWL4PQWUDCACHL/graph.json","events_json":"https://pith.science/api/pith-number/7TESLSNF6FRCPWL4PQWUDCACHL/events.json","paper":"https://pith.science/paper/7TESLSNF"},"agent_actions":{"view_html":"https://pith.science/pith/7TESLSNF6FRCPWL4PQWUDCACHL","download_json":"https://pith.science/pith/7TESLSNF6FRCPWL4PQWUDCACHL.json","view_paper":"https://pith.science/paper/7TESLSNF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.28115&json=true","fetch_graph":"https://pith.science/api/pith-number/7TESLSNF6FRCPWL4PQWUDCACHL/graph.json","fetch_events":"https://pith.science/api/pith-number/7TESLSNF6FRCPWL4PQWUDCACHL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7TESLSNF6FRCPWL4PQWUDCACHL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7TESLSNF6FRCPWL4PQWUDCACHL/action/storage_attestation","attest_author":"https://pith.science/pith/7TESLSNF6FRCPWL4PQWUDCACHL/action/author_attestation","sign_citation":"https://pith.science/pith/7TESLSNF6FRCPWL4PQWUDCACHL/action/citation_signature","submit_replication":"https://pith.science/pith/7TESLSNF6FRCPWL4PQWUDCACHL/action/replication_record"}},"created_at":"2026-06-29T01:15:06.460573+00:00","updated_at":"2026-06-29T01:15:06.460573+00:00"}