{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:IOTDXKCMHEGADDY2B7PIXJLYLY","short_pith_number":"pith:IOTDXKCM","schema_version":"1.0","canonical_sha256":"43a63ba84c390c018f1a0fde8ba5785e191713769e36aed3ec1b55c2e5bfe631","source":{"kind":"arxiv","id":"1304.4129","version":1},"attestation_state":"computed","paper":{"title":"The hybrid B-type pulsator $\\gamma$ Pegasi: mode identification and complex seismic modelling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Alexey A. Pamyatnykh, Jadwiga Daszy\\'nska-Daszkiewicz, Przemys{\\l}aw Walczak, Tomasz Zdravkov","submitted_at":"2013-04-15T15:23:38Z","abstract_excerpt":"We present interpretation of the oscillation spectrum of the early B-type star $\\gamma$ Pegasi, in which both low order p/g and high-order g-modes are observed. Using amplitudes and phases of the photometric and radial velocity variations, we identify/constrain the mode degree, $\\ell$, for all 14 detected frequencies. Seismic models fitting two pulsational frequencies corresponding to the modes $\\ell=0$, p$_1$ and $\\ell=1$, g$_1$ were constructed. This set of models contains those which reproduce also the empirical values of the complex nonadiabatic parameter $f$ associated to these two mode f"},"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":"1304.4129","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-04-15T15:23:38Z","cross_cats_sorted":[],"title_canon_sha256":"324ea37fd318cd373bbe3f3f04f1276b4fa4e1e9d649ef6b9d737c1bfd4c58ad","abstract_canon_sha256":"110b1398c03f4c79f61a934c1b7815607f1e825b11f46f0b904b08f7203e5c95"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:50:32.693945Z","signature_b64":"DkDotvYBHkadzFwMYEswVKJ7fma+OSlqLJuS3Wh1uJL0MqUxvt8/y5/Li9dnfw5KvmrmnG7mKpFtj+t5H8WaCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"43a63ba84c390c018f1a0fde8ba5785e191713769e36aed3ec1b55c2e5bfe631","last_reissued_at":"2026-05-18T01:50:32.693359Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:50:32.693359Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The hybrid B-type pulsator $\\gamma$ Pegasi: mode identification and complex seismic modelling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Alexey A. Pamyatnykh, Jadwiga Daszy\\'nska-Daszkiewicz, Przemys{\\l}aw Walczak, Tomasz Zdravkov","submitted_at":"2013-04-15T15:23:38Z","abstract_excerpt":"We present interpretation of the oscillation spectrum of the early B-type star $\\gamma$ Pegasi, in which both low order p/g and high-order g-modes are observed. Using amplitudes and phases of the photometric and radial velocity variations, we identify/constrain the mode degree, $\\ell$, for all 14 detected frequencies. Seismic models fitting two pulsational frequencies corresponding to the modes $\\ell=0$, p$_1$ and $\\ell=1$, g$_1$ were constructed. This set of models contains those which reproduce also the empirical values of the complex nonadiabatic parameter $f$ associated to these two mode f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1304.4129","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":"1304.4129","created_at":"2026-05-18T01:50:32.693455+00:00"},{"alias_kind":"arxiv_version","alias_value":"1304.4129v1","created_at":"2026-05-18T01:50:32.693455+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1304.4129","created_at":"2026-05-18T01:50:32.693455+00:00"},{"alias_kind":"pith_short_12","alias_value":"IOTDXKCMHEGA","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_16","alias_value":"IOTDXKCMHEGADDY2","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_8","alias_value":"IOTDXKCM","created_at":"2026-05-18T12:27:46.883200+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/IOTDXKCMHEGADDY2B7PIXJLYLY","json":"https://pith.science/pith/IOTDXKCMHEGADDY2B7PIXJLYLY.json","graph_json":"https://pith.science/api/pith-number/IOTDXKCMHEGADDY2B7PIXJLYLY/graph.json","events_json":"https://pith.science/api/pith-number/IOTDXKCMHEGADDY2B7PIXJLYLY/events.json","paper":"https://pith.science/paper/IOTDXKCM"},"agent_actions":{"view_html":"https://pith.science/pith/IOTDXKCMHEGADDY2B7PIXJLYLY","download_json":"https://pith.science/pith/IOTDXKCMHEGADDY2B7PIXJLYLY.json","view_paper":"https://pith.science/paper/IOTDXKCM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1304.4129&json=true","fetch_graph":"https://pith.science/api/pith-number/IOTDXKCMHEGADDY2B7PIXJLYLY/graph.json","fetch_events":"https://pith.science/api/pith-number/IOTDXKCMHEGADDY2B7PIXJLYLY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IOTDXKCMHEGADDY2B7PIXJLYLY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IOTDXKCMHEGADDY2B7PIXJLYLY/action/storage_attestation","attest_author":"https://pith.science/pith/IOTDXKCMHEGADDY2B7PIXJLYLY/action/author_attestation","sign_citation":"https://pith.science/pith/IOTDXKCMHEGADDY2B7PIXJLYLY/action/citation_signature","submit_replication":"https://pith.science/pith/IOTDXKCMHEGADDY2B7PIXJLYLY/action/replication_record"}},"created_at":"2026-05-18T01:50:32.693455+00:00","updated_at":"2026-05-18T01:50:32.693455+00:00"}