{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:64Y6H5BIMVHQAIX63AR45B3S6U","short_pith_number":"pith:64Y6H5BI","schema_version":"1.0","canonical_sha256":"f731e3f428654f0022fed823ce8772f524bff6111e836defccfc9ea0e6e9688b","source":{"kind":"arxiv","id":"2606.00209","version":1},"attestation_state":"computed","paper":{"title":"On the Faint Early-time Radio and X-ray Emissions in TDE2025aarm","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Tatsuya Matsumoto, Tsvi Piran","submitted_at":"2026-05-29T18:00:00Z","abstract_excerpt":"TDE2025aarm is a nearby tidal disruption event whose early radio and X-ray emissions are exceptionally faint compared with previously observed TDEs. We examine whether these weak signals can be explained within standard outflow and disk-emission scenarios. The radio detection at $15\\,\\rm GHz$ with $\\sim10^{36}\\,\\rm erg\\,s^{-1}$ around $40\\,\\rm days$ after discovery is inconsistent with synchrotron emission from a quasi-spherical disk wind for reasonable circum-nuclear densities and outflow velocities. Instead, the low luminosity and inferred self-absorbed spectrum imply a narrowly collimated o"},"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":"2606.00209","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-05-29T18:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"275ddc63bdcb0badef498e5df7f8e6cc808a80b92001ce9955a8b84541295d7e","abstract_canon_sha256":"14a6449ce74c914b557a6731ced5b884f7e69a4df6f5e87613a142b6ed6b1da4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-02T01:03:21.661792Z","signature_b64":"Y47O6GT+ZDkkMvDbiQpghkgyLV5ONtaoj+Nl5C5veYEFu1fo+3omzxeFEzDeYhQwV/irNzRedM4YMniUvhg3Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f731e3f428654f0022fed823ce8772f524bff6111e836defccfc9ea0e6e9688b","last_reissued_at":"2026-06-02T01:03:21.661444Z","signature_status":"signed_v1","first_computed_at":"2026-06-02T01:03:21.661444Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the Faint Early-time Radio and X-ray Emissions in TDE2025aarm","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Tatsuya Matsumoto, Tsvi Piran","submitted_at":"2026-05-29T18:00:00Z","abstract_excerpt":"TDE2025aarm is a nearby tidal disruption event whose early radio and X-ray emissions are exceptionally faint compared with previously observed TDEs. We examine whether these weak signals can be explained within standard outflow and disk-emission scenarios. The radio detection at $15\\,\\rm GHz$ with $\\sim10^{36}\\,\\rm erg\\,s^{-1}$ around $40\\,\\rm days$ after discovery is inconsistent with synchrotron emission from a quasi-spherical disk wind for reasonable circum-nuclear densities and outflow velocities. Instead, the low luminosity and inferred self-absorbed spectrum imply a narrowly collimated o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.00209","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/2606.00209/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":"2606.00209","created_at":"2026-06-02T01:03:21.661500+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.00209v1","created_at":"2026-06-02T01:03:21.661500+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.00209","created_at":"2026-06-02T01:03:21.661500+00:00"},{"alias_kind":"pith_short_12","alias_value":"64Y6H5BIMVHQ","created_at":"2026-06-02T01:03:21.661500+00:00"},{"alias_kind":"pith_short_16","alias_value":"64Y6H5BIMVHQAIX6","created_at":"2026-06-02T01:03:21.661500+00:00"},{"alias_kind":"pith_short_8","alias_value":"64Y6H5BI","created_at":"2026-06-02T01:03:21.661500+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/64Y6H5BIMVHQAIX63AR45B3S6U","json":"https://pith.science/pith/64Y6H5BIMVHQAIX63AR45B3S6U.json","graph_json":"https://pith.science/api/pith-number/64Y6H5BIMVHQAIX63AR45B3S6U/graph.json","events_json":"https://pith.science/api/pith-number/64Y6H5BIMVHQAIX63AR45B3S6U/events.json","paper":"https://pith.science/paper/64Y6H5BI"},"agent_actions":{"view_html":"https://pith.science/pith/64Y6H5BIMVHQAIX63AR45B3S6U","download_json":"https://pith.science/pith/64Y6H5BIMVHQAIX63AR45B3S6U.json","view_paper":"https://pith.science/paper/64Y6H5BI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.00209&json=true","fetch_graph":"https://pith.science/api/pith-number/64Y6H5BIMVHQAIX63AR45B3S6U/graph.json","fetch_events":"https://pith.science/api/pith-number/64Y6H5BIMVHQAIX63AR45B3S6U/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/64Y6H5BIMVHQAIX63AR45B3S6U/action/timestamp_anchor","attest_storage":"https://pith.science/pith/64Y6H5BIMVHQAIX63AR45B3S6U/action/storage_attestation","attest_author":"https://pith.science/pith/64Y6H5BIMVHQAIX63AR45B3S6U/action/author_attestation","sign_citation":"https://pith.science/pith/64Y6H5BIMVHQAIX63AR45B3S6U/action/citation_signature","submit_replication":"https://pith.science/pith/64Y6H5BIMVHQAIX63AR45B3S6U/action/replication_record"}},"created_at":"2026-06-02T01:03:21.661500+00:00","updated_at":"2026-06-02T01:03:21.661500+00:00"}