{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:B5TT56QSS3LETKYMH7D6BTV3EE","short_pith_number":"pith:B5TT56QS","schema_version":"1.0","canonical_sha256":"0f673efa1296d649ab0c3fc7e0cebb2116be61796b9c801b7306c99d818c2df2","source":{"kind":"arxiv","id":"1403.7155","version":2},"attestation_state":"computed","paper":{"title":"Rotation and magnetism of Kepler pulsating solar-like stars. Towards asteroseismically calibrated age-rotation relations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Jimenez, C. Karoff, D. Salabert, G.R. Davies, J. Ballot, J.C. Suarez, J.-D. do Nascimento Jr., J.L. van Saders, M.B. Nielsen, M. Pinsonneault, P.G. Beck, R.A. Garcia, S. Bloemen, S. Mathis, S. Mathur, T. Ceillier, T.L. Campante, T.S. Metcalfe, W.J. Chaplin","submitted_at":"2014-03-27T18:05:47Z","abstract_excerpt":"Kepler ultra-high precision photometry of long and continuous observations provides a unique dataset in which surface rotation and variability can be studied for thousands of stars. Because many of these old field stars also have independently measured asteroseismic ages, measurements of rotation and activity are particularly interesting in the context of age-rotation-activity relations. In particular, age-rotation relations generally lack good calibrators at old ages, a problem that this Kepler sample of old-field stars is uniquely suited to address. We study the surface rotation and photomet"},"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":"1403.7155","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-03-27T18:05:47Z","cross_cats_sorted":[],"title_canon_sha256":"f53c26c155b42230dd422ca4b1a09d72f902c493faf88727d3c1d1c92ea52f9f","abstract_canon_sha256":"0071da429d4473b33649eb0cf49982e4b0c0ef38a221690f470eab6c35eeddb0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:32:54.060093Z","signature_b64":"J/22uc40rYCzgGf1ER/G/pdj3AH3FYJIOBVDKWCf4RdMoGX8xb8qZVFBniEO10W+FdkgJGWH19T2SQOA+4RRBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0f673efa1296d649ab0c3fc7e0cebb2116be61796b9c801b7306c99d818c2df2","last_reissued_at":"2026-05-18T02:32:54.059673Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:32:54.059673Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Rotation and magnetism of Kepler pulsating solar-like stars. Towards asteroseismically calibrated age-rotation relations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Jimenez, C. Karoff, D. Salabert, G.R. Davies, J. Ballot, J.C. Suarez, J.-D. do Nascimento Jr., J.L. van Saders, M.B. Nielsen, M. Pinsonneault, P.G. Beck, R.A. Garcia, S. Bloemen, S. Mathis, S. Mathur, T. Ceillier, T.L. Campante, T.S. Metcalfe, W.J. Chaplin","submitted_at":"2014-03-27T18:05:47Z","abstract_excerpt":"Kepler ultra-high precision photometry of long and continuous observations provides a unique dataset in which surface rotation and variability can be studied for thousands of stars. Because many of these old field stars also have independently measured asteroseismic ages, measurements of rotation and activity are particularly interesting in the context of age-rotation-activity relations. In particular, age-rotation relations generally lack good calibrators at old ages, a problem that this Kepler sample of old-field stars is uniquely suited to address. We study the surface rotation and photomet"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.7155","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":"1403.7155","created_at":"2026-05-18T02:32:54.059739+00:00"},{"alias_kind":"arxiv_version","alias_value":"1403.7155v2","created_at":"2026-05-18T02:32:54.059739+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.7155","created_at":"2026-05-18T02:32:54.059739+00:00"},{"alias_kind":"pith_short_12","alias_value":"B5TT56QSS3LE","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_16","alias_value":"B5TT56QSS3LETKYM","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_8","alias_value":"B5TT56QS","created_at":"2026-05-18T12:28:22.404517+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1906.12262","citing_title":"Asteroseismology of solar-type stars","ref_index":196,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/B5TT56QSS3LETKYMH7D6BTV3EE","json":"https://pith.science/pith/B5TT56QSS3LETKYMH7D6BTV3EE.json","graph_json":"https://pith.science/api/pith-number/B5TT56QSS3LETKYMH7D6BTV3EE/graph.json","events_json":"https://pith.science/api/pith-number/B5TT56QSS3LETKYMH7D6BTV3EE/events.json","paper":"https://pith.science/paper/B5TT56QS"},"agent_actions":{"view_html":"https://pith.science/pith/B5TT56QSS3LETKYMH7D6BTV3EE","download_json":"https://pith.science/pith/B5TT56QSS3LETKYMH7D6BTV3EE.json","view_paper":"https://pith.science/paper/B5TT56QS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1403.7155&json=true","fetch_graph":"https://pith.science/api/pith-number/B5TT56QSS3LETKYMH7D6BTV3EE/graph.json","fetch_events":"https://pith.science/api/pith-number/B5TT56QSS3LETKYMH7D6BTV3EE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/B5TT56QSS3LETKYMH7D6BTV3EE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/B5TT56QSS3LETKYMH7D6BTV3EE/action/storage_attestation","attest_author":"https://pith.science/pith/B5TT56QSS3LETKYMH7D6BTV3EE/action/author_attestation","sign_citation":"https://pith.science/pith/B5TT56QSS3LETKYMH7D6BTV3EE/action/citation_signature","submit_replication":"https://pith.science/pith/B5TT56QSS3LETKYMH7D6BTV3EE/action/replication_record"}},"created_at":"2026-05-18T02:32:54.059739+00:00","updated_at":"2026-05-18T02:32:54.059739+00:00"}