{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:UZ2NONYDH4JW5CEGNBQJRY47CH","short_pith_number":"pith:UZ2NONYD","schema_version":"1.0","canonical_sha256":"a674d737033f136e8886686098e39f11ccb31bbc20b38c2e62081c6d01ec98dc","source":{"kind":"arxiv","id":"2406.08012","version":4},"attestation_state":"computed","paper":{"title":"Interaction of an outflow with surrounding gaseous clouds as the origin of the late-time radio flares in TDEs","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Guobin Mou, Jialun Zhuang, Rong-Feng Shen, Wenbin Lu","submitted_at":"2024-06-12T09:04:12Z","abstract_excerpt":"Close encounter between a star and a supermassive black hole (SMBH) results in the tidal disruption of the star, known as a tidal disruption event (TDE). Recently, a few TDEs, e.g., ASASSN-15oi and AT2018hyz, have shown late-time (hundreds of days after their UV/optical peaks) radio flares with radio luminosities of $10^{38\\sim39}$ erg/s. The super-Eddington fallback or accretion in a TDE may generate a mass outflow. Here we investigate a scenario that the late-time radio flares come from the interaction of the outflow with the circum-nuclear gaseous clouds, in addition to the slow-evolving em"},"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":"2406.08012","kind":"arxiv","version":4},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-06-12T09:04:12Z","cross_cats_sorted":[],"title_canon_sha256":"d9b2dc73ff6e7dfa9052fe29d444ce7991ba188b4bd4f96fc5a0a9fe2dcc932a","abstract_canon_sha256":"c9b7466c409c129109d8a2f7d3a8ebcf5b117602666a4a622135b0f05ed13113"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:50:27.124565Z","signature_b64":"cd/ab9KJravwdNQL/HZEU1bxMBqH9af9MNNYhZu8cp5KIn1UZW6Fv5dgy+yKrRyTtF5At/N9fLUi3wAm0t4CCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a674d737033f136e8886686098e39f11ccb31bbc20b38c2e62081c6d01ec98dc","last_reissued_at":"2026-07-05T11:50:27.124045Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:50:27.124045Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Interaction of an outflow with surrounding gaseous clouds as the origin of the late-time radio flares in TDEs","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Guobin Mou, Jialun Zhuang, Rong-Feng Shen, Wenbin Lu","submitted_at":"2024-06-12T09:04:12Z","abstract_excerpt":"Close encounter between a star and a supermassive black hole (SMBH) results in the tidal disruption of the star, known as a tidal disruption event (TDE). Recently, a few TDEs, e.g., ASASSN-15oi and AT2018hyz, have shown late-time (hundreds of days after their UV/optical peaks) radio flares with radio luminosities of $10^{38\\sim39}$ erg/s. The super-Eddington fallback or accretion in a TDE may generate a mass outflow. Here we investigate a scenario that the late-time radio flares come from the interaction of the outflow with the circum-nuclear gaseous clouds, in addition to the slow-evolving em"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2406.08012","kind":"arxiv","version":4},"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/2406.08012/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":"2406.08012","created_at":"2026-07-05T11:50:27.124105+00:00"},{"alias_kind":"arxiv_version","alias_value":"2406.08012v4","created_at":"2026-07-05T11:50:27.124105+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2406.08012","created_at":"2026-07-05T11:50:27.124105+00:00"},{"alias_kind":"pith_short_12","alias_value":"UZ2NONYDH4JW","created_at":"2026-07-05T11:50:27.124105+00:00"},{"alias_kind":"pith_short_16","alias_value":"UZ2NONYDH4JW5CEG","created_at":"2026-07-05T11:50:27.124105+00:00"},{"alias_kind":"pith_short_8","alias_value":"UZ2NONYD","created_at":"2026-07-05T11:50:27.124105+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.01273","citing_title":"Radio emission from tidal disruption events produced by the collision between super-Eddington outflows and the circumnuclear medium","ref_index":74,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UZ2NONYDH4JW5CEGNBQJRY47CH","json":"https://pith.science/pith/UZ2NONYDH4JW5CEGNBQJRY47CH.json","graph_json":"https://pith.science/api/pith-number/UZ2NONYDH4JW5CEGNBQJRY47CH/graph.json","events_json":"https://pith.science/api/pith-number/UZ2NONYDH4JW5CEGNBQJRY47CH/events.json","paper":"https://pith.science/paper/UZ2NONYD"},"agent_actions":{"view_html":"https://pith.science/pith/UZ2NONYDH4JW5CEGNBQJRY47CH","download_json":"https://pith.science/pith/UZ2NONYDH4JW5CEGNBQJRY47CH.json","view_paper":"https://pith.science/paper/UZ2NONYD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2406.08012&json=true","fetch_graph":"https://pith.science/api/pith-number/UZ2NONYDH4JW5CEGNBQJRY47CH/graph.json","fetch_events":"https://pith.science/api/pith-number/UZ2NONYDH4JW5CEGNBQJRY47CH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UZ2NONYDH4JW5CEGNBQJRY47CH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UZ2NONYDH4JW5CEGNBQJRY47CH/action/storage_attestation","attest_author":"https://pith.science/pith/UZ2NONYDH4JW5CEGNBQJRY47CH/action/author_attestation","sign_citation":"https://pith.science/pith/UZ2NONYDH4JW5CEGNBQJRY47CH/action/citation_signature","submit_replication":"https://pith.science/pith/UZ2NONYDH4JW5CEGNBQJRY47CH/action/replication_record"}},"created_at":"2026-07-05T11:50:27.124105+00:00","updated_at":"2026-07-05T11:50:27.124105+00:00"}