{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:PR5BLKQMAOUBWEWVTHAE55HZP6","short_pith_number":"pith:PR5BLKQM","schema_version":"1.0","canonical_sha256":"7c7a15aa0c03a81b12d599c04ef4f97fb15047d0d894ed3fd759fe5af434952a","source":{"kind":"arxiv","id":"1004.2366","version":2},"attestation_state":"computed","paper":{"title":"Complex asteroseismology of the hybrid B-type pulsator $\\gamma$ Pegasi: a test of stellar opacities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Jadwiga Daszy\\'nska-Daszkiewicz, Przemys{\\l}aw Walczak","submitted_at":"2010-04-14T10:38:47Z","abstract_excerpt":"Using the updated oscillation spectrum of $\\gamma$ Pegasi, we construct a set of seismic models which reproduce two pulsational frequencies corresponding to the $\\ell=0$, p$_1$ and $\\ell=1$, g$_1$ modes. Then, we single out models which reproduce other well identified modes. Finally, we extend our seismic modelling by a requirement of fitting also values of the complex, nonadiabatic parameter $f$ associated to each mode frequency. Such complex asteroseismology of the B-type pulsators provides a unique test of stellar metallicity and opacities. In contrast to our previous studies, results for $"},"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":"1004.2366","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-04-14T10:38:47Z","cross_cats_sorted":[],"title_canon_sha256":"2f7ec88bf23c67ff4888b6c616caa1dbd87682756dcb15d0ee6b202dd86af1eb","abstract_canon_sha256":"bad1896864398757928a6fafb44bffdfc0cb9306bc04f9401c9cfc2c653053a1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:08:05.798599Z","signature_b64":"7ao0OCLpZKCq/kkhMOU+FRRWYLkcpC0/Fb+zsfQrB9DCvv9cvCdudQUO10wIPwcLqFP59fOS8HXl7PzysW4DCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7c7a15aa0c03a81b12d599c04ef4f97fb15047d0d894ed3fd759fe5af434952a","last_reissued_at":"2026-05-18T02:08:05.797802Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:08:05.797802Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Complex asteroseismology of the hybrid B-type pulsator $\\gamma$ Pegasi: a test of stellar opacities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Jadwiga Daszy\\'nska-Daszkiewicz, Przemys{\\l}aw Walczak","submitted_at":"2010-04-14T10:38:47Z","abstract_excerpt":"Using the updated oscillation spectrum of $\\gamma$ Pegasi, we construct a set of seismic models which reproduce two pulsational frequencies corresponding to the $\\ell=0$, p$_1$ and $\\ell=1$, g$_1$ modes. Then, we single out models which reproduce other well identified modes. Finally, we extend our seismic modelling by a requirement of fitting also values of the complex, nonadiabatic parameter $f$ associated to each mode frequency. Such complex asteroseismology of the B-type pulsators provides a unique test of stellar metallicity and opacities. In contrast to our previous studies, results for $"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1004.2366","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":"1004.2366","created_at":"2026-05-18T02:08:05.797936+00:00"},{"alias_kind":"arxiv_version","alias_value":"1004.2366v2","created_at":"2026-05-18T02:08:05.797936+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1004.2366","created_at":"2026-05-18T02:08:05.797936+00:00"},{"alias_kind":"pith_short_12","alias_value":"PR5BLKQMAOUB","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_16","alias_value":"PR5BLKQMAOUBWEWV","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_8","alias_value":"PR5BLKQM","created_at":"2026-05-18T12:26:12.377268+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/PR5BLKQMAOUBWEWVTHAE55HZP6","json":"https://pith.science/pith/PR5BLKQMAOUBWEWVTHAE55HZP6.json","graph_json":"https://pith.science/api/pith-number/PR5BLKQMAOUBWEWVTHAE55HZP6/graph.json","events_json":"https://pith.science/api/pith-number/PR5BLKQMAOUBWEWVTHAE55HZP6/events.json","paper":"https://pith.science/paper/PR5BLKQM"},"agent_actions":{"view_html":"https://pith.science/pith/PR5BLKQMAOUBWEWVTHAE55HZP6","download_json":"https://pith.science/pith/PR5BLKQMAOUBWEWVTHAE55HZP6.json","view_paper":"https://pith.science/paper/PR5BLKQM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1004.2366&json=true","fetch_graph":"https://pith.science/api/pith-number/PR5BLKQMAOUBWEWVTHAE55HZP6/graph.json","fetch_events":"https://pith.science/api/pith-number/PR5BLKQMAOUBWEWVTHAE55HZP6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PR5BLKQMAOUBWEWVTHAE55HZP6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PR5BLKQMAOUBWEWVTHAE55HZP6/action/storage_attestation","attest_author":"https://pith.science/pith/PR5BLKQMAOUBWEWVTHAE55HZP6/action/author_attestation","sign_citation":"https://pith.science/pith/PR5BLKQMAOUBWEWVTHAE55HZP6/action/citation_signature","submit_replication":"https://pith.science/pith/PR5BLKQMAOUBWEWVTHAE55HZP6/action/replication_record"}},"created_at":"2026-05-18T02:08:05.797936+00:00","updated_at":"2026-05-18T02:08:05.797936+00:00"}