{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:7232A4NOLMVSTBWORSUX4OMLFU","short_pith_number":"pith:7232A4NO","schema_version":"1.0","canonical_sha256":"feb7a071ae5b2b2986ce8ca97e398b2d119a06656512478a7fcb3a1affd0672b","source":{"kind":"arxiv","id":"1610.06184","version":2},"attestation_state":"computed","paper":{"title":"A new asteroseismic diagnostic for internal rotation in $\\gamma$ Doradus stars","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"I. W. Roxburgh, Rhita-Maria Ouazzani, S.J.A.J. Salmon, S. J. Murphy, T. R. Bedding, V. Antoci","submitted_at":"2016-10-19T20:00:05Z","abstract_excerpt":"With four years of nearly-continuous photometry from Kepler, we are finally in a good position to apply asteroseismology to $\\gamma$ Doradus stars. In particular several analyses have demonstrated the possibility to detect non-uniform period spacings, which have been predicted to be directly related to rotation. In the present work, we define a new seismic diagnostic for rotation in $\\gamma$ Doradus stars that are too rapidly rotating to present rotational splittings. Based on the non uniformity of their period spacings, we define the observable $\\Sigma$ as the slope of the period spacing when"},"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":"1610.06184","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-19T20:00:05Z","cross_cats_sorted":[],"title_canon_sha256":"4d818daca791a31d51cf2a226bcd90bb92f22e0350582e43d7e467c8599afc2b","abstract_canon_sha256":"21c5d53880192dd0c360c281aa0ffcb1e586d33a2904844d837b4671245958d1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:52:38.304520Z","signature_b64":"mxS1Q/I4B/OHY/I6X4Ei2JsBfff2hW7LZRKNXn3Gnhc0izz2ZSh27qB4btCjciR7L/epq/+zVT1QEYAKQINaCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"feb7a071ae5b2b2986ce8ca97e398b2d119a06656512478a7fcb3a1affd0672b","last_reissued_at":"2026-05-18T00:52:38.303999Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:52:38.303999Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A new asteroseismic diagnostic for internal rotation in $\\gamma$ Doradus stars","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"I. W. Roxburgh, Rhita-Maria Ouazzani, S.J.A.J. Salmon, S. J. Murphy, T. R. Bedding, V. Antoci","submitted_at":"2016-10-19T20:00:05Z","abstract_excerpt":"With four years of nearly-continuous photometry from Kepler, we are finally in a good position to apply asteroseismology to $\\gamma$ Doradus stars. In particular several analyses have demonstrated the possibility to detect non-uniform period spacings, which have been predicted to be directly related to rotation. In the present work, we define a new seismic diagnostic for rotation in $\\gamma$ Doradus stars that are too rapidly rotating to present rotational splittings. Based on the non uniformity of their period spacings, we define the observable $\\Sigma$ as the slope of the period spacing when"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.06184","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":"1610.06184","created_at":"2026-05-18T00:52:38.304073+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.06184v2","created_at":"2026-05-18T00:52:38.304073+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.06184","created_at":"2026-05-18T00:52:38.304073+00:00"},{"alias_kind":"pith_short_12","alias_value":"7232A4NOLMVS","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_16","alias_value":"7232A4NOLMVSTBWO","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_8","alias_value":"7232A4NO","created_at":"2026-05-18T12:30:04.600751+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.22533","citing_title":"Seismic signature of a magnetic field in the $\\gamma$ Doradus star KIC 2309579","ref_index":10,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7232A4NOLMVSTBWORSUX4OMLFU","json":"https://pith.science/pith/7232A4NOLMVSTBWORSUX4OMLFU.json","graph_json":"https://pith.science/api/pith-number/7232A4NOLMVSTBWORSUX4OMLFU/graph.json","events_json":"https://pith.science/api/pith-number/7232A4NOLMVSTBWORSUX4OMLFU/events.json","paper":"https://pith.science/paper/7232A4NO"},"agent_actions":{"view_html":"https://pith.science/pith/7232A4NOLMVSTBWORSUX4OMLFU","download_json":"https://pith.science/pith/7232A4NOLMVSTBWORSUX4OMLFU.json","view_paper":"https://pith.science/paper/7232A4NO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.06184&json=true","fetch_graph":"https://pith.science/api/pith-number/7232A4NOLMVSTBWORSUX4OMLFU/graph.json","fetch_events":"https://pith.science/api/pith-number/7232A4NOLMVSTBWORSUX4OMLFU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7232A4NOLMVSTBWORSUX4OMLFU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7232A4NOLMVSTBWORSUX4OMLFU/action/storage_attestation","attest_author":"https://pith.science/pith/7232A4NOLMVSTBWORSUX4OMLFU/action/author_attestation","sign_citation":"https://pith.science/pith/7232A4NOLMVSTBWORSUX4OMLFU/action/citation_signature","submit_replication":"https://pith.science/pith/7232A4NOLMVSTBWORSUX4OMLFU/action/replication_record"}},"created_at":"2026-05-18T00:52:38.304073+00:00","updated_at":"2026-05-18T00:52:38.304073+00:00"}