{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:ZHWKJQODGGJRH77A7EP77BPSP7","short_pith_number":"pith:ZHWKJQOD","schema_version":"1.0","canonical_sha256":"c9eca4c1c3319313ffe0f91fff85f27ff6ab03c06b20d093d1bd33b9f6f84e46","source":{"kind":"arxiv","id":"2504.12762","version":4},"attestation_state":"computed","paper":{"title":"Testing the Shock-cooling Emission Model from Star-Disk Collisions for Quasiperiodic Eruptions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.SR","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Rong-Feng Shen (SYSU), Wenyuan Guo (SYSU)","submitted_at":"2025-04-17T09:00:00Z","abstract_excerpt":"Quasiperiodic eruptions (QPEs), the repeated outbursts observed in soft X-ray bands, have attracted broad interest, but their physical origin is under debate. One of the popular models, the star-disk collision model, suggests that QPEs can be produced through periodic collisions of an orbiting star with the accretion disk of a central black hole (BH). However, previous tests of the star-disk collision model mainly focus on the timing analysis. Other observed properties, such as peak luminosities $L_{\\rm{p}}$, durations $t_{\\rm{e}}$, and radiation temperatures $T_{\\rm{p}}$ of the eruptions, are"},"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":"2504.12762","kind":"arxiv","version":4},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-04-17T09:00:00Z","cross_cats_sorted":["astro-ph.GA","astro-ph.SR","hep-ph"],"title_canon_sha256":"8ed1d98fbf9b359c9e30bf83401a68ad5bb3817b251b6427d1f221300b2365c8","abstract_canon_sha256":"4488f92ae07671155460373afad1c3dff8035b0ce5a3436d3830e2460bc038c7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-02T02:04:05.714365Z","signature_b64":"jN5EUvlT25BiP1SQP0ltatd6dCHECfYLzAEDkZ2RLsRgCve4U8/lkCMZKQR0CHHqxQPEsX1bvH7DxqSCxVWACg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c9eca4c1c3319313ffe0f91fff85f27ff6ab03c06b20d093d1bd33b9f6f84e46","last_reissued_at":"2026-06-02T02:04:05.713886Z","signature_status":"signed_v1","first_computed_at":"2026-06-02T02:04:05.713886Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Testing the Shock-cooling Emission Model from Star-Disk Collisions for Quasiperiodic Eruptions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.SR","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Rong-Feng Shen (SYSU), Wenyuan Guo (SYSU)","submitted_at":"2025-04-17T09:00:00Z","abstract_excerpt":"Quasiperiodic eruptions (QPEs), the repeated outbursts observed in soft X-ray bands, have attracted broad interest, but their physical origin is under debate. One of the popular models, the star-disk collision model, suggests that QPEs can be produced through periodic collisions of an orbiting star with the accretion disk of a central black hole (BH). However, previous tests of the star-disk collision model mainly focus on the timing analysis. Other observed properties, such as peak luminosities $L_{\\rm{p}}$, durations $t_{\\rm{e}}$, and radiation temperatures $T_{\\rm{p}}$ of the eruptions, are"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2504.12762","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/2504.12762/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":"2504.12762","created_at":"2026-06-02T02:04:05.713948+00:00"},{"alias_kind":"arxiv_version","alias_value":"2504.12762v4","created_at":"2026-06-02T02:04:05.713948+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2504.12762","created_at":"2026-06-02T02:04:05.713948+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZHWKJQODGGJR","created_at":"2026-06-02T02:04:05.713948+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZHWKJQODGGJRH77A","created_at":"2026-06-02T02:04:05.713948+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZHWKJQOD","created_at":"2026-06-02T02:04:05.713948+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2604.09788","citing_title":"Even a precessing clock is right twice per orbit -- The super-periods of eRO-QPE2 and challenges for quasi-periodic eruption orbital models","ref_index":30,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZHWKJQODGGJRH77A7EP77BPSP7","json":"https://pith.science/pith/ZHWKJQODGGJRH77A7EP77BPSP7.json","graph_json":"https://pith.science/api/pith-number/ZHWKJQODGGJRH77A7EP77BPSP7/graph.json","events_json":"https://pith.science/api/pith-number/ZHWKJQODGGJRH77A7EP77BPSP7/events.json","paper":"https://pith.science/paper/ZHWKJQOD"},"agent_actions":{"view_html":"https://pith.science/pith/ZHWKJQODGGJRH77A7EP77BPSP7","download_json":"https://pith.science/pith/ZHWKJQODGGJRH77A7EP77BPSP7.json","view_paper":"https://pith.science/paper/ZHWKJQOD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2504.12762&json=true","fetch_graph":"https://pith.science/api/pith-number/ZHWKJQODGGJRH77A7EP77BPSP7/graph.json","fetch_events":"https://pith.science/api/pith-number/ZHWKJQODGGJRH77A7EP77BPSP7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZHWKJQODGGJRH77A7EP77BPSP7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZHWKJQODGGJRH77A7EP77BPSP7/action/storage_attestation","attest_author":"https://pith.science/pith/ZHWKJQODGGJRH77A7EP77BPSP7/action/author_attestation","sign_citation":"https://pith.science/pith/ZHWKJQODGGJRH77A7EP77BPSP7/action/citation_signature","submit_replication":"https://pith.science/pith/ZHWKJQODGGJRH77A7EP77BPSP7/action/replication_record"}},"created_at":"2026-06-02T02:04:05.713948+00:00","updated_at":"2026-06-02T02:04:05.713948+00:00"}