{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:TUYMQHHHH2GLD3UJ5H4CUHSDVO","short_pith_number":"pith:TUYMQHHH","schema_version":"1.0","canonical_sha256":"9d30c81ce73e8cb1ee89e9f82a1e43ab9892e5686d6cb2a0aedac9e6d4da4e13","source":{"kind":"arxiv","id":"1108.0857","version":1},"attestation_state":"computed","paper":{"title":"Spectroscopic monitoring of the Herbig Ae star HD 104237. II. Non-radial pulsations, mode analysis and fundamental stellar parameters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Aurelie Fumel, Torsten Boehm","submitted_at":"2011-08-03T14:49:12Z","abstract_excerpt":"Herbig Ae/Be stars are intermediate-mass pre-main sequence (PMS) stars showing signs of intense activity and strong stellar winds, whose origin is not yet understood in the frame of current theoretical models of stellar evolution for young stars. The evolutionary tracks of the earlier Herbig Ae stars cross a recently discovered PMS instability strip. Many of these stars exhibit pulsations of delta Scuti type. HD 104237 is a well-known pulsating Herbig Ae star. In this article, we reinvestigated an extensive high-resolution quasi-continuous spectroscopic data set in order to search for very fai"},"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":"1108.0857","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-08-03T14:49:12Z","cross_cats_sorted":[],"title_canon_sha256":"5e210b4cd79a6f9259139aff7443e6ea1fe9fb6708ee71b7197534c5b772aacc","abstract_canon_sha256":"ece3785448b2b3ef6c355ac234d26bf17d2f5820e1cac00c04c9454274c47a87"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:03.539248Z","signature_b64":"UPOsUcPBfm/nVn6WAscL+xfybp6a24uFyT+Wyo4SHHokyZxZk01+11SJIVVzRcdU/WakwGm6M7DT77zvprSuCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9d30c81ce73e8cb1ee89e9f82a1e43ab9892e5686d6cb2a0aedac9e6d4da4e13","last_reissued_at":"2026-05-18T02:01:03.538523Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:03.538523Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spectroscopic monitoring of the Herbig Ae star HD 104237. II. Non-radial pulsations, mode analysis and fundamental stellar parameters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Aurelie Fumel, Torsten Boehm","submitted_at":"2011-08-03T14:49:12Z","abstract_excerpt":"Herbig Ae/Be stars are intermediate-mass pre-main sequence (PMS) stars showing signs of intense activity and strong stellar winds, whose origin is not yet understood in the frame of current theoretical models of stellar evolution for young stars. The evolutionary tracks of the earlier Herbig Ae stars cross a recently discovered PMS instability strip. Many of these stars exhibit pulsations of delta Scuti type. HD 104237 is a well-known pulsating Herbig Ae star. In this article, we reinvestigated an extensive high-resolution quasi-continuous spectroscopic data set in order to search for very fai"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.0857","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":"1108.0857","created_at":"2026-05-18T02:01:03.538648+00:00"},{"alias_kind":"arxiv_version","alias_value":"1108.0857v1","created_at":"2026-05-18T02:01:03.538648+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.0857","created_at":"2026-05-18T02:01:03.538648+00:00"},{"alias_kind":"pith_short_12","alias_value":"TUYMQHHHH2GL","created_at":"2026-05-18T12:26:42.757692+00:00"},{"alias_kind":"pith_short_16","alias_value":"TUYMQHHHH2GLD3UJ","created_at":"2026-05-18T12:26:42.757692+00:00"},{"alias_kind":"pith_short_8","alias_value":"TUYMQHHH","created_at":"2026-05-18T12:26:42.757692+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/TUYMQHHHH2GLD3UJ5H4CUHSDVO","json":"https://pith.science/pith/TUYMQHHHH2GLD3UJ5H4CUHSDVO.json","graph_json":"https://pith.science/api/pith-number/TUYMQHHHH2GLD3UJ5H4CUHSDVO/graph.json","events_json":"https://pith.science/api/pith-number/TUYMQHHHH2GLD3UJ5H4CUHSDVO/events.json","paper":"https://pith.science/paper/TUYMQHHH"},"agent_actions":{"view_html":"https://pith.science/pith/TUYMQHHHH2GLD3UJ5H4CUHSDVO","download_json":"https://pith.science/pith/TUYMQHHHH2GLD3UJ5H4CUHSDVO.json","view_paper":"https://pith.science/paper/TUYMQHHH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1108.0857&json=true","fetch_graph":"https://pith.science/api/pith-number/TUYMQHHHH2GLD3UJ5H4CUHSDVO/graph.json","fetch_events":"https://pith.science/api/pith-number/TUYMQHHHH2GLD3UJ5H4CUHSDVO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TUYMQHHHH2GLD3UJ5H4CUHSDVO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TUYMQHHHH2GLD3UJ5H4CUHSDVO/action/storage_attestation","attest_author":"https://pith.science/pith/TUYMQHHHH2GLD3UJ5H4CUHSDVO/action/author_attestation","sign_citation":"https://pith.science/pith/TUYMQHHHH2GLD3UJ5H4CUHSDVO/action/citation_signature","submit_replication":"https://pith.science/pith/TUYMQHHHH2GLD3UJ5H4CUHSDVO/action/replication_record"}},"created_at":"2026-05-18T02:01:03.538648+00:00","updated_at":"2026-05-18T02:01:03.538648+00:00"}