{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:5WQKDZ32T5S25CUOGHSYIIVSEI","short_pith_number":"pith:5WQKDZ32","schema_version":"1.0","canonical_sha256":"eda0a1e77a9f65ae8a8e31e58422b22220644064e9cf48b1f19eca7a05c6342e","source":{"kind":"arxiv","id":"1405.0739","version":1},"attestation_state":"computed","paper":{"title":"A Strict Test of Stellar Evolution Models: The Absolute Dimensions of Massive Benchmark Eclipsing Binary V578 Mon","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Claret, E.V. Garcia, H. Hensberge, Keivan G. Stassun, K. Pavlovski, Y. G\\'omez Maqueo Chew","submitted_at":"2014-05-04T20:36:03Z","abstract_excerpt":"We determine the absolute dimensions of the eclipsing binary V578 Mon, a detached system of two early B-type stars (B0V + B1V, P$=$2.40848 d) in the star-forming region NGC 2244 of the Rosette Nebula. From the light curve analysis of 40 yr of photometry and the analysis of HERMES spectra, we find radii of $5.41\\pm0.04$ Rsun and $4.29\\pm 0.05$ Rsun, and temperatures of $ 30000\\pm 500$~K and $ 25750\\pm 435$ K respectively. We find that our disentangled component spectra for V578 Mon agree well previous spectral disentangling from the literature. We also reconfirm the previous spectroscopic orbit"},"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":"1405.0739","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-05-04T20:36:03Z","cross_cats_sorted":[],"title_canon_sha256":"7b840bee0d10dc018e91d1ab9f3b852d5d6fd159a091ad386c4534bd15cf2b55","abstract_canon_sha256":"7862a22b085207f8b670db4c9c37dd4e14aae8b5cf52aa36e6c3eec5f5cfb4f5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:18.112694Z","signature_b64":"WD/3/GETAQS/sNRB13IxV9CLwruBOTBMFhGrAhqj7PjLON8zJyjvsPY5TN4p7x3BixN3l0soInwjd2oCxC0yBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"eda0a1e77a9f65ae8a8e31e58422b22220644064e9cf48b1f19eca7a05c6342e","last_reissued_at":"2026-05-18T01:43:18.111978Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:18.111978Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Strict Test of Stellar Evolution Models: The Absolute Dimensions of Massive Benchmark Eclipsing Binary V578 Mon","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Claret, E.V. Garcia, H. Hensberge, Keivan G. Stassun, K. Pavlovski, Y. G\\'omez Maqueo Chew","submitted_at":"2014-05-04T20:36:03Z","abstract_excerpt":"We determine the absolute dimensions of the eclipsing binary V578 Mon, a detached system of two early B-type stars (B0V + B1V, P$=$2.40848 d) in the star-forming region NGC 2244 of the Rosette Nebula. From the light curve analysis of 40 yr of photometry and the analysis of HERMES spectra, we find radii of $5.41\\pm0.04$ Rsun and $4.29\\pm 0.05$ Rsun, and temperatures of $ 30000\\pm 500$~K and $ 25750\\pm 435$ K respectively. We find that our disentangled component spectra for V578 Mon agree well previous spectral disentangling from the literature. We also reconfirm the previous spectroscopic orbit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.0739","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":"1405.0739","created_at":"2026-05-18T01:43:18.112111+00:00"},{"alias_kind":"arxiv_version","alias_value":"1405.0739v1","created_at":"2026-05-18T01:43:18.112111+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.0739","created_at":"2026-05-18T01:43:18.112111+00:00"},{"alias_kind":"pith_short_12","alias_value":"5WQKDZ32T5S2","created_at":"2026-05-18T12:28:16.859392+00:00"},{"alias_kind":"pith_short_16","alias_value":"5WQKDZ32T5S25CUO","created_at":"2026-05-18T12:28:16.859392+00:00"},{"alias_kind":"pith_short_8","alias_value":"5WQKDZ32","created_at":"2026-05-18T12:28:16.859392+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/5WQKDZ32T5S25CUOGHSYIIVSEI","json":"https://pith.science/pith/5WQKDZ32T5S25CUOGHSYIIVSEI.json","graph_json":"https://pith.science/api/pith-number/5WQKDZ32T5S25CUOGHSYIIVSEI/graph.json","events_json":"https://pith.science/api/pith-number/5WQKDZ32T5S25CUOGHSYIIVSEI/events.json","paper":"https://pith.science/paper/5WQKDZ32"},"agent_actions":{"view_html":"https://pith.science/pith/5WQKDZ32T5S25CUOGHSYIIVSEI","download_json":"https://pith.science/pith/5WQKDZ32T5S25CUOGHSYIIVSEI.json","view_paper":"https://pith.science/paper/5WQKDZ32","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1405.0739&json=true","fetch_graph":"https://pith.science/api/pith-number/5WQKDZ32T5S25CUOGHSYIIVSEI/graph.json","fetch_events":"https://pith.science/api/pith-number/5WQKDZ32T5S25CUOGHSYIIVSEI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5WQKDZ32T5S25CUOGHSYIIVSEI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5WQKDZ32T5S25CUOGHSYIIVSEI/action/storage_attestation","attest_author":"https://pith.science/pith/5WQKDZ32T5S25CUOGHSYIIVSEI/action/author_attestation","sign_citation":"https://pith.science/pith/5WQKDZ32T5S25CUOGHSYIIVSEI/action/citation_signature","submit_replication":"https://pith.science/pith/5WQKDZ32T5S25CUOGHSYIIVSEI/action/replication_record"}},"created_at":"2026-05-18T01:43:18.112111+00:00","updated_at":"2026-05-18T01:43:18.112111+00:00"}