{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:G6XGOPQVMD5SNGEK5TP4XYUWQP","short_pith_number":"pith:G6XGOPQV","schema_version":"1.0","canonical_sha256":"37ae673e1560fb26988aecdfcbe29683c2e1b1037ca23a26eacdd682fba28751","source":{"kind":"arxiv","id":"1506.08902","version":1},"attestation_state":"computed","paper":{"title":"Modeling the Complete Lightcurve of omega CMa","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A.C. Carciofi, A.T. Okazaki, D.Baade, J.E. Bjorkman, L.R. Rimulo, M.R. Ghoreyshi, S. Otero, Th. Rivinius","submitted_at":"2015-06-29T23:57:53Z","abstract_excerpt":"We have used the radiative transfer code HDUST to analyze and interpret the long-term photometric behavior of the Be star omega CMa, considering four complete cycles of disk formation and dissipation. This is the first time in which a full lightcurve of a Be star was investigated and modeled including both disk build-up and dissipation phases. Based on the quite good fit of the observed data we were able to derive the history of stellar mass decretion rates (including long- and short-term changes) during the disk formation and dissipation phases in all four cycles."},"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":"1506.08902","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-06-29T23:57:53Z","cross_cats_sorted":[],"title_canon_sha256":"b30a64b3b8ede48525c5fd7b1c9dcb57f6f055dc19ebb3d1422534c4e8cace5e","abstract_canon_sha256":"fbaeeb95176bd24bac6d3ab4badb1e4ca7b6daadf22205b36d070ad2696d8040"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:37:34.167452Z","signature_b64":"kzdEUw0Ut2tQCqZ58NG+HnxH7DZ4OYWbctf/WELVQ4ZyQVRhakHSeKyerurqDREOmmMhyK/zUh1rfvK/UyteCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"37ae673e1560fb26988aecdfcbe29683c2e1b1037ca23a26eacdd682fba28751","last_reissued_at":"2026-05-18T01:37:34.166598Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:37:34.166598Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Modeling the Complete Lightcurve of omega CMa","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A.C. Carciofi, A.T. Okazaki, D.Baade, J.E. Bjorkman, L.R. Rimulo, M.R. Ghoreyshi, S. Otero, Th. Rivinius","submitted_at":"2015-06-29T23:57:53Z","abstract_excerpt":"We have used the radiative transfer code HDUST to analyze and interpret the long-term photometric behavior of the Be star omega CMa, considering four complete cycles of disk formation and dissipation. This is the first time in which a full lightcurve of a Be star was investigated and modeled including both disk build-up and dissipation phases. Based on the quite good fit of the observed data we were able to derive the history of stellar mass decretion rates (including long- and short-term changes) during the disk formation and dissipation phases in all four cycles."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.08902","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":"1506.08902","created_at":"2026-05-18T01:37:34.166760+00:00"},{"alias_kind":"arxiv_version","alias_value":"1506.08902v1","created_at":"2026-05-18T01:37:34.166760+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.08902","created_at":"2026-05-18T01:37:34.166760+00:00"},{"alias_kind":"pith_short_12","alias_value":"G6XGOPQVMD5S","created_at":"2026-05-18T12:29:22.688609+00:00"},{"alias_kind":"pith_short_16","alias_value":"G6XGOPQVMD5SNGEK","created_at":"2026-05-18T12:29:22.688609+00:00"},{"alias_kind":"pith_short_8","alias_value":"G6XGOPQV","created_at":"2026-05-18T12:29:22.688609+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/G6XGOPQVMD5SNGEK5TP4XYUWQP","json":"https://pith.science/pith/G6XGOPQVMD5SNGEK5TP4XYUWQP.json","graph_json":"https://pith.science/api/pith-number/G6XGOPQVMD5SNGEK5TP4XYUWQP/graph.json","events_json":"https://pith.science/api/pith-number/G6XGOPQVMD5SNGEK5TP4XYUWQP/events.json","paper":"https://pith.science/paper/G6XGOPQV"},"agent_actions":{"view_html":"https://pith.science/pith/G6XGOPQVMD5SNGEK5TP4XYUWQP","download_json":"https://pith.science/pith/G6XGOPQVMD5SNGEK5TP4XYUWQP.json","view_paper":"https://pith.science/paper/G6XGOPQV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1506.08902&json=true","fetch_graph":"https://pith.science/api/pith-number/G6XGOPQVMD5SNGEK5TP4XYUWQP/graph.json","fetch_events":"https://pith.science/api/pith-number/G6XGOPQVMD5SNGEK5TP4XYUWQP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G6XGOPQVMD5SNGEK5TP4XYUWQP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G6XGOPQVMD5SNGEK5TP4XYUWQP/action/storage_attestation","attest_author":"https://pith.science/pith/G6XGOPQVMD5SNGEK5TP4XYUWQP/action/author_attestation","sign_citation":"https://pith.science/pith/G6XGOPQVMD5SNGEK5TP4XYUWQP/action/citation_signature","submit_replication":"https://pith.science/pith/G6XGOPQVMD5SNGEK5TP4XYUWQP/action/replication_record"}},"created_at":"2026-05-18T01:37:34.166760+00:00","updated_at":"2026-05-18T01:37:34.166760+00:00"}