{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:LEV26YPLKANVS6U55M3EV2K6JP","short_pith_number":"pith:LEV26YPL","schema_version":"1.0","canonical_sha256":"592baf61eb501b597a9deb364ae95e4bd8ba142a047e5d80e1369bf2145721ea","source":{"kind":"arxiv","id":"1708.05088","version":2},"attestation_state":"computed","paper":{"title":"Stellar population of the superbubble N206 in the LMC I. Analysis of the Of-type stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"A. A. C. Sander, H. Todt, J. S. Gallagher, L. M. Oskinova, R. Hainich, T. Shenar, Varsha Ramachandran, W.-R. Hamann","submitted_at":"2017-08-16T21:27:59Z","abstract_excerpt":"Massive stars are the key agents of feedback. Consequently, quantitative analysis of massive stars are required to understand how the feedback of these objects shapes/ creates the large scale structures of the ISM. The giant HII region N206 in the Large Magellanic Cloud contains an OB association that powers a X-ray superbubble, serving as an ideal laboratory in this context. We obtained optical spectra with the muti-object spectrograph FLAMES at the ESO-VLT. When possible, the optical spectroscopy was complemented by UV spectra from the HST, IUE, and FUSE archives. Detailed spectral classific"},"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":"1708.05088","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-08-16T21:27:59Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"9212d9a036445e5fb0d836f1ab558c9cfa6e249f8dc7fa4d2d4b01ef6d0e10bb","abstract_canon_sha256":"2cbe0fa7d1cc2bcda6472362abb89b6da692ea43a348b0d1da12efe0236901f2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:27:13.147030Z","signature_b64":"ytjoWBSPHYECSJzs49HCbxf9B1Gk4a0GWtApjPQKHv4PpR5F0GGfDoctvtBRbZa1pgSDppOLXpDtaegM//NtCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"592baf61eb501b597a9deb364ae95e4bd8ba142a047e5d80e1369bf2145721ea","last_reissued_at":"2026-05-18T00:27:13.146474Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:27:13.146474Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stellar population of the superbubble N206 in the LMC I. Analysis of the Of-type stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"A. A. C. Sander, H. Todt, J. S. Gallagher, L. M. Oskinova, R. Hainich, T. Shenar, Varsha Ramachandran, W.-R. Hamann","submitted_at":"2017-08-16T21:27:59Z","abstract_excerpt":"Massive stars are the key agents of feedback. Consequently, quantitative analysis of massive stars are required to understand how the feedback of these objects shapes/ creates the large scale structures of the ISM. The giant HII region N206 in the Large Magellanic Cloud contains an OB association that powers a X-ray superbubble, serving as an ideal laboratory in this context. We obtained optical spectra with the muti-object spectrograph FLAMES at the ESO-VLT. When possible, the optical spectroscopy was complemented by UV spectra from the HST, IUE, and FUSE archives. Detailed spectral classific"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.05088","kind":"arxiv","version":2},"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":"1708.05088","created_at":"2026-05-18T00:27:13.146549+00:00"},{"alias_kind":"arxiv_version","alias_value":"1708.05088v2","created_at":"2026-05-18T00:27:13.146549+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.05088","created_at":"2026-05-18T00:27:13.146549+00:00"},{"alias_kind":"pith_short_12","alias_value":"LEV26YPLKANV","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_16","alias_value":"LEV26YPLKANVS6U5","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_8","alias_value":"LEV26YPL","created_at":"2026-05-18T12:31:28.150371+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/LEV26YPLKANVS6U55M3EV2K6JP","json":"https://pith.science/pith/LEV26YPLKANVS6U55M3EV2K6JP.json","graph_json":"https://pith.science/api/pith-number/LEV26YPLKANVS6U55M3EV2K6JP/graph.json","events_json":"https://pith.science/api/pith-number/LEV26YPLKANVS6U55M3EV2K6JP/events.json","paper":"https://pith.science/paper/LEV26YPL"},"agent_actions":{"view_html":"https://pith.science/pith/LEV26YPLKANVS6U55M3EV2K6JP","download_json":"https://pith.science/pith/LEV26YPLKANVS6U55M3EV2K6JP.json","view_paper":"https://pith.science/paper/LEV26YPL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1708.05088&json=true","fetch_graph":"https://pith.science/api/pith-number/LEV26YPLKANVS6U55M3EV2K6JP/graph.json","fetch_events":"https://pith.science/api/pith-number/LEV26YPLKANVS6U55M3EV2K6JP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LEV26YPLKANVS6U55M3EV2K6JP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LEV26YPLKANVS6U55M3EV2K6JP/action/storage_attestation","attest_author":"https://pith.science/pith/LEV26YPLKANVS6U55M3EV2K6JP/action/author_attestation","sign_citation":"https://pith.science/pith/LEV26YPLKANVS6U55M3EV2K6JP/action/citation_signature","submit_replication":"https://pith.science/pith/LEV26YPLKANVS6U55M3EV2K6JP/action/replication_record"}},"created_at":"2026-05-18T00:27:13.146549+00:00","updated_at":"2026-05-18T00:27:13.146549+00:00"}