{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:CTNJILG6AVU64G2TFIUULC6QCX","short_pith_number":"pith:CTNJILG6","schema_version":"1.0","canonical_sha256":"14da942cde0569ee1b532a29458bd015c3f39fa5e7f34ec3af4db553430ec0f2","source":{"kind":"arxiv","id":"1802.07494","version":2},"attestation_state":"computed","paper":{"title":"Stellar population of the superbubble N206 in the LMC II. Parameters of the OB and WR stars, and the total massive star feedback","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","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":"2018-02-21T10:20:15Z","abstract_excerpt":"Clusters or associations of early-type stars are often associated with a 'superbubble' of hot gas. The formation of such superbubbles is caused by the feedback from massive stars. The complex N206 in the Large Magellanic Cloud exhibits a superbubble and a rich massive star population. We observed these massive stars using the FLAMES multi-object spectrograph at ESO-VLT. Available UV spectra from HST, IUE, and FUSE are also used. The spectral analysis is performed with Potsdam Wolf-Rayet (PoWR) model atmospheres. We present the stellar and wind parameters of the OB stars and the two WR binaries"},"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":"1802.07494","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-02-21T10:20:15Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"ddee39ec0d2304b220997bcaf90dcea62c01be695a5a0c2d9d24262e8dc95c74","abstract_canon_sha256":"91afd2bdfc2e4f93eb73045053aacc33468b192863c4a8bce2bc9950a335dd15"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:10:31.769875Z","signature_b64":"MEhA37OZ/7HM5LseArxz3kobT7qGPB4l03nh7yzyuIf4hyjyTn4DY7XxE3LXIS2MmZ1K0iKRGjiTAk/UovGrBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"14da942cde0569ee1b532a29458bd015c3f39fa5e7f34ec3af4db553430ec0f2","last_reissued_at":"2026-05-18T00:10:31.769278Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:10:31.769278Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stellar population of the superbubble N206 in the LMC II. Parameters of the OB and WR stars, and the total massive star feedback","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","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":"2018-02-21T10:20:15Z","abstract_excerpt":"Clusters or associations of early-type stars are often associated with a 'superbubble' of hot gas. The formation of such superbubbles is caused by the feedback from massive stars. The complex N206 in the Large Magellanic Cloud exhibits a superbubble and a rich massive star population. We observed these massive stars using the FLAMES multi-object spectrograph at ESO-VLT. Available UV spectra from HST, IUE, and FUSE are also used. The spectral analysis is performed with Potsdam Wolf-Rayet (PoWR) model atmospheres. We present the stellar and wind parameters of the OB stars and the two WR binaries"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.07494","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":"1802.07494","created_at":"2026-05-18T00:10:31.769374+00:00"},{"alias_kind":"arxiv_version","alias_value":"1802.07494v2","created_at":"2026-05-18T00:10:31.769374+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.07494","created_at":"2026-05-18T00:10:31.769374+00:00"},{"alias_kind":"pith_short_12","alias_value":"CTNJILG6AVU6","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_16","alias_value":"CTNJILG6AVU64G2T","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_8","alias_value":"CTNJILG6","created_at":"2026-05-18T12:32:19.392346+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/CTNJILG6AVU64G2TFIUULC6QCX","json":"https://pith.science/pith/CTNJILG6AVU64G2TFIUULC6QCX.json","graph_json":"https://pith.science/api/pith-number/CTNJILG6AVU64G2TFIUULC6QCX/graph.json","events_json":"https://pith.science/api/pith-number/CTNJILG6AVU64G2TFIUULC6QCX/events.json","paper":"https://pith.science/paper/CTNJILG6"},"agent_actions":{"view_html":"https://pith.science/pith/CTNJILG6AVU64G2TFIUULC6QCX","download_json":"https://pith.science/pith/CTNJILG6AVU64G2TFIUULC6QCX.json","view_paper":"https://pith.science/paper/CTNJILG6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1802.07494&json=true","fetch_graph":"https://pith.science/api/pith-number/CTNJILG6AVU64G2TFIUULC6QCX/graph.json","fetch_events":"https://pith.science/api/pith-number/CTNJILG6AVU64G2TFIUULC6QCX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CTNJILG6AVU64G2TFIUULC6QCX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CTNJILG6AVU64G2TFIUULC6QCX/action/storage_attestation","attest_author":"https://pith.science/pith/CTNJILG6AVU64G2TFIUULC6QCX/action/author_attestation","sign_citation":"https://pith.science/pith/CTNJILG6AVU64G2TFIUULC6QCX/action/citation_signature","submit_replication":"https://pith.science/pith/CTNJILG6AVU64G2TFIUULC6QCX/action/replication_record"}},"created_at":"2026-05-18T00:10:31.769374+00:00","updated_at":"2026-05-18T00:10:31.769374+00:00"}