{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:SSBOBL3L6PQGSXCA6IDW6CWD2N","short_pith_number":"pith:SSBOBL3L","schema_version":"1.0","canonical_sha256":"9482e0af6bf3e0695c40f2076f0ac3d36217f0c329b7aab130ab8eb12c9b505b","source":{"kind":"arxiv","id":"1803.00243","version":1},"attestation_state":"computed","paper":{"title":"Fundamental parameters of massive stars in multiple systems: The cases of HD17505A and HD206267A","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"F. Raucq, G. Rauw, L. Mahy, S. Sim\\'on-D\\'iaz","submitted_at":"2018-03-01T08:21:46Z","abstract_excerpt":"Many massive stars are part of binary or higher multiplicity systems. The present work focusses on two higher multiplicity systems: HD17505A and HD206267A. Determining the fundamental parameters of the components of the inner binary of these systems is mandatory to quantify the impact of binary or triple interactions on their evolution. We analysed high-resolution optical spectra to determine new orbital solutions of the inner binary systems. After subtracting the spectrum of the tertiary component, a spectral disentangling code was applied to reconstruct the individual spectra of the primary "},"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":"1803.00243","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-03-01T08:21:46Z","cross_cats_sorted":[],"title_canon_sha256":"ae99c42d6cd1753f099058cead033a27e942f8cfc976acd83846a08cc2a4bd66","abstract_canon_sha256":"f183e24f5e941b2a3bee7a5aa27fbd10257fd181df77da88e6a3657826384d23"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:13:27.380858Z","signature_b64":"5Pm6/Xku2nBhlS8R4C+DgNDe4h3Olua4nrsMFSgt1M5k8RRRqwihww5lcHKqeZ7yAHa/X3yYo8drPGh+yLalBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9482e0af6bf3e0695c40f2076f0ac3d36217f0c329b7aab130ab8eb12c9b505b","last_reissued_at":"2026-05-18T00:13:27.380060Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:13:27.380060Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fundamental parameters of massive stars in multiple systems: The cases of HD17505A and HD206267A","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"F. Raucq, G. Rauw, L. Mahy, S. Sim\\'on-D\\'iaz","submitted_at":"2018-03-01T08:21:46Z","abstract_excerpt":"Many massive stars are part of binary or higher multiplicity systems. The present work focusses on two higher multiplicity systems: HD17505A and HD206267A. Determining the fundamental parameters of the components of the inner binary of these systems is mandatory to quantify the impact of binary or triple interactions on their evolution. We analysed high-resolution optical spectra to determine new orbital solutions of the inner binary systems. After subtracting the spectrum of the tertiary component, a spectral disentangling code was applied to reconstruct the individual spectra of the primary "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1803.00243","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":""},"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":"1803.00243","created_at":"2026-05-18T00:13:27.380219+00:00"},{"alias_kind":"arxiv_version","alias_value":"1803.00243v1","created_at":"2026-05-18T00:13:27.380219+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1803.00243","created_at":"2026-05-18T00:13:27.380219+00:00"},{"alias_kind":"pith_short_12","alias_value":"SSBOBL3L6PQG","created_at":"2026-05-18T12:32:53.628368+00:00"},{"alias_kind":"pith_short_16","alias_value":"SSBOBL3L6PQGSXCA","created_at":"2026-05-18T12:32:53.628368+00:00"},{"alias_kind":"pith_short_8","alias_value":"SSBOBL3L","created_at":"2026-05-18T12:32:53.628368+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/SSBOBL3L6PQGSXCA6IDW6CWD2N","json":"https://pith.science/pith/SSBOBL3L6PQGSXCA6IDW6CWD2N.json","graph_json":"https://pith.science/api/pith-number/SSBOBL3L6PQGSXCA6IDW6CWD2N/graph.json","events_json":"https://pith.science/api/pith-number/SSBOBL3L6PQGSXCA6IDW6CWD2N/events.json","paper":"https://pith.science/paper/SSBOBL3L"},"agent_actions":{"view_html":"https://pith.science/pith/SSBOBL3L6PQGSXCA6IDW6CWD2N","download_json":"https://pith.science/pith/SSBOBL3L6PQGSXCA6IDW6CWD2N.json","view_paper":"https://pith.science/paper/SSBOBL3L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1803.00243&json=true","fetch_graph":"https://pith.science/api/pith-number/SSBOBL3L6PQGSXCA6IDW6CWD2N/graph.json","fetch_events":"https://pith.science/api/pith-number/SSBOBL3L6PQGSXCA6IDW6CWD2N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SSBOBL3L6PQGSXCA6IDW6CWD2N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SSBOBL3L6PQGSXCA6IDW6CWD2N/action/storage_attestation","attest_author":"https://pith.science/pith/SSBOBL3L6PQGSXCA6IDW6CWD2N/action/author_attestation","sign_citation":"https://pith.science/pith/SSBOBL3L6PQGSXCA6IDW6CWD2N/action/citation_signature","submit_replication":"https://pith.science/pith/SSBOBL3L6PQGSXCA6IDW6CWD2N/action/replication_record"}},"created_at":"2026-05-18T00:13:27.380219+00:00","updated_at":"2026-05-18T00:13:27.380219+00:00"}