{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:JQAY7LPG2KFTMIQFTZ7FFR22FZ","short_pith_number":"pith:JQAY7LPG","schema_version":"1.0","canonical_sha256":"4c018fade6d28b3622059e7e52c75a2e4a3d4af7b573278ce135b81d2fd91b2c","source":{"kind":"arxiv","id":"2212.09599","version":1},"attestation_state":"computed","paper":{"title":"Impact of tides on non-coplanar orbits of progenitors of high-mass X-ray binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"A. Simaz Bunzel, F. Fortin, F. Garc\\'ia, J. A. Combi, S. Chaty","submitted_at":"2022-12-19T16:35:38Z","abstract_excerpt":"An important stage in the evolution of massive binaries is the formation of a compact object in the system. It is believed that in some cases a momentum kick is imparted to the newly born object, changing the orbital parameters of the binary, such as eccentricity and orbital period, and even acquiring an asynchronous orbit between its components. In this situation, tides play a central role in the evolution of these binaries. In this work we aim to study how the orbital parameters of a massive binary change after the formation of a compact object when the stellar spin of the non-degenerate com"},"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":"2212.09599","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2022-12-19T16:35:38Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"de9b3ae52defd48baa290e0070bf3420aa190e0d184eb941f07baef8c9b9f199","abstract_canon_sha256":"3afd60dd97b1d3a65540b3693d3340a33dcd84759a646f5b317ff3f3a86c0563"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:38:22.382743Z","signature_b64":"tGljI618Z9wINsBejh2E0dBQO7gcXv81ORaoQbpprUbbGQwMcM5OaYLHbixboSbRyb5rxm/QpqVqTViwknWlDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4c018fade6d28b3622059e7e52c75a2e4a3d4af7b573278ce135b81d2fd91b2c","last_reissued_at":"2026-07-05T05:38:22.382265Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:38:22.382265Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Impact of tides on non-coplanar orbits of progenitors of high-mass X-ray binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"A. Simaz Bunzel, F. Fortin, F. Garc\\'ia, J. A. Combi, S. Chaty","submitted_at":"2022-12-19T16:35:38Z","abstract_excerpt":"An important stage in the evolution of massive binaries is the formation of a compact object in the system. It is believed that in some cases a momentum kick is imparted to the newly born object, changing the orbital parameters of the binary, such as eccentricity and orbital period, and even acquiring an asynchronous orbit between its components. In this situation, tides play a central role in the evolution of these binaries. In this work we aim to study how the orbital parameters of a massive binary change after the formation of a compact object when the stellar spin of the non-degenerate com"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2212.09599","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/2212.09599/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":"2212.09599","created_at":"2026-07-05T05:38:22.382322+00:00"},{"alias_kind":"arxiv_version","alias_value":"2212.09599v1","created_at":"2026-07-05T05:38:22.382322+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2212.09599","created_at":"2026-07-05T05:38:22.382322+00:00"},{"alias_kind":"pith_short_12","alias_value":"JQAY7LPG2KFT","created_at":"2026-07-05T05:38:22.382322+00:00"},{"alias_kind":"pith_short_16","alias_value":"JQAY7LPG2KFTMIQF","created_at":"2026-07-05T05:38:22.382322+00:00"},{"alias_kind":"pith_short_8","alias_value":"JQAY7LPG","created_at":"2026-07-05T05:38:22.382322+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/JQAY7LPG2KFTMIQFTZ7FFR22FZ","json":"https://pith.science/pith/JQAY7LPG2KFTMIQFTZ7FFR22FZ.json","graph_json":"https://pith.science/api/pith-number/JQAY7LPG2KFTMIQFTZ7FFR22FZ/graph.json","events_json":"https://pith.science/api/pith-number/JQAY7LPG2KFTMIQFTZ7FFR22FZ/events.json","paper":"https://pith.science/paper/JQAY7LPG"},"agent_actions":{"view_html":"https://pith.science/pith/JQAY7LPG2KFTMIQFTZ7FFR22FZ","download_json":"https://pith.science/pith/JQAY7LPG2KFTMIQFTZ7FFR22FZ.json","view_paper":"https://pith.science/paper/JQAY7LPG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2212.09599&json=true","fetch_graph":"https://pith.science/api/pith-number/JQAY7LPG2KFTMIQFTZ7FFR22FZ/graph.json","fetch_events":"https://pith.science/api/pith-number/JQAY7LPG2KFTMIQFTZ7FFR22FZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JQAY7LPG2KFTMIQFTZ7FFR22FZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JQAY7LPG2KFTMIQFTZ7FFR22FZ/action/storage_attestation","attest_author":"https://pith.science/pith/JQAY7LPG2KFTMIQFTZ7FFR22FZ/action/author_attestation","sign_citation":"https://pith.science/pith/JQAY7LPG2KFTMIQFTZ7FFR22FZ/action/citation_signature","submit_replication":"https://pith.science/pith/JQAY7LPG2KFTMIQFTZ7FFR22FZ/action/replication_record"}},"created_at":"2026-07-05T05:38:22.382322+00:00","updated_at":"2026-07-05T05:38:22.382322+00:00"}