{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:JOKQSO6UGNLVPD3EMKP67Q6TD3","short_pith_number":"pith:JOKQSO6U","schema_version":"1.0","canonical_sha256":"4b95093bd43357578f64629fefc3d31ed2d483dce13ac9b09c385fa292f354ff","source":{"kind":"arxiv","id":"2508.14161","version":1},"attestation_state":"computed","paper":{"title":"Minimum and maximum mass-luminosity relations for stripped stars","license":"http://creativecommons.org/licenses/by-sa/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Andreas A. C. Sander, Gautham N. Sabhahit, Jorick S. Vink, Varsha Ramachandran","submitted_at":"2025-08-19T18:00:02Z","abstract_excerpt":"Envelope stripping, whether through single-star wind mass loss or binary mass transfer, is a key evolutionary pathway for the formation of classical Wolf-Rayet stars and lower-mass stripped helium (He) stars. However, to study the evolution of these objects into black holes, neutron stars, and stripped-envelope supernovae, we need appropriate input models for the core-He burning phase without relying on the uncertain evolution into this evolved phase. Reliable mass-luminosity relations (MLRs) for He stars are needed for stellar wind and evolution studies, but the MLRs currently in literature a"},"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":"2508.14161","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-sa/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2025-08-19T18:00:02Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"3a3dc2fac02077cecc4a6596f4fe2f03d462ba7ff23dc28358047cf9eb2e1ec1","abstract_canon_sha256":"b7651d55ed7c8b731cb8de702aff47200175ce86d46f7874e630677d4caa292d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:56:26.728450Z","signature_b64":"V2og30VIeE9QdpkYsASjOe9w5X237CKH+AyUwnDfVfmN3U2wRhG9w4UsIQdfCYNqdkxt7uK7+7GFxsD7Ll9BCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4b95093bd43357578f64629fefc3d31ed2d483dce13ac9b09c385fa292f354ff","last_reissued_at":"2026-07-05T11:56:26.727962Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:56:26.727962Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Minimum and maximum mass-luminosity relations for stripped stars","license":"http://creativecommons.org/licenses/by-sa/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Andreas A. C. Sander, Gautham N. Sabhahit, Jorick S. Vink, Varsha Ramachandran","submitted_at":"2025-08-19T18:00:02Z","abstract_excerpt":"Envelope stripping, whether through single-star wind mass loss or binary mass transfer, is a key evolutionary pathway for the formation of classical Wolf-Rayet stars and lower-mass stripped helium (He) stars. However, to study the evolution of these objects into black holes, neutron stars, and stripped-envelope supernovae, we need appropriate input models for the core-He burning phase without relying on the uncertain evolution into this evolved phase. Reliable mass-luminosity relations (MLRs) for He stars are needed for stellar wind and evolution studies, but the MLRs currently in literature a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2508.14161","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/2508.14161/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":"2508.14161","created_at":"2026-07-05T11:56:26.728019+00:00"},{"alias_kind":"arxiv_version","alias_value":"2508.14161v1","created_at":"2026-07-05T11:56:26.728019+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2508.14161","created_at":"2026-07-05T11:56:26.728019+00:00"},{"alias_kind":"pith_short_12","alias_value":"JOKQSO6UGNLV","created_at":"2026-07-05T11:56:26.728019+00:00"},{"alias_kind":"pith_short_16","alias_value":"JOKQSO6UGNLVPD3E","created_at":"2026-07-05T11:56:26.728019+00:00"},{"alias_kind":"pith_short_8","alias_value":"JOKQSO6U","created_at":"2026-07-05T11:56:26.728019+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/JOKQSO6UGNLVPD3EMKP67Q6TD3","json":"https://pith.science/pith/JOKQSO6UGNLVPD3EMKP67Q6TD3.json","graph_json":"https://pith.science/api/pith-number/JOKQSO6UGNLVPD3EMKP67Q6TD3/graph.json","events_json":"https://pith.science/api/pith-number/JOKQSO6UGNLVPD3EMKP67Q6TD3/events.json","paper":"https://pith.science/paper/JOKQSO6U"},"agent_actions":{"view_html":"https://pith.science/pith/JOKQSO6UGNLVPD3EMKP67Q6TD3","download_json":"https://pith.science/pith/JOKQSO6UGNLVPD3EMKP67Q6TD3.json","view_paper":"https://pith.science/paper/JOKQSO6U","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2508.14161&json=true","fetch_graph":"https://pith.science/api/pith-number/JOKQSO6UGNLVPD3EMKP67Q6TD3/graph.json","fetch_events":"https://pith.science/api/pith-number/JOKQSO6UGNLVPD3EMKP67Q6TD3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JOKQSO6UGNLVPD3EMKP67Q6TD3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JOKQSO6UGNLVPD3EMKP67Q6TD3/action/storage_attestation","attest_author":"https://pith.science/pith/JOKQSO6UGNLVPD3EMKP67Q6TD3/action/author_attestation","sign_citation":"https://pith.science/pith/JOKQSO6UGNLVPD3EMKP67Q6TD3/action/citation_signature","submit_replication":"https://pith.science/pith/JOKQSO6UGNLVPD3EMKP67Q6TD3/action/replication_record"}},"created_at":"2026-07-05T11:56:26.728019+00:00","updated_at":"2026-07-05T11:56:26.728019+00:00"}