{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:NPJQQSHHZ3BRS6EKR6JOUSCJ7N","short_pith_number":"pith:NPJQQSHH","schema_version":"1.0","canonical_sha256":"6bd30848e7cec319788a8f92ea4849fb456dbca2acddf46b7b22c9b269a77606","source":{"kind":"arxiv","id":"1307.4218","version":1},"attestation_state":"computed","paper":{"title":"Bayesian Asteroseismology of 23 Solar-Like Kepler Targets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"David B. Guenther, Kieran MacLeod, Michael Gruberbauer, Thomas Kallinger","submitted_at":"2013-07-16T09:38:57Z","abstract_excerpt":"We study 23 previously published Kepler targets to perform a consistent grid-based Bayesian asteroseismic analysis and compare our results to those obtained via the Asteroseismic Modelling Portal (AMP). We find differences in the derived stellar parameters of many targets and their uncertainties. While some of these differences can be attributed to systematic effects between stellar evolutionary models, we show that the different methodologies deliver incompatible uncertainties for some parameters. Using non-adiabatic models and our capability to measure surface effects, we also investigate th"},"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":"1307.4218","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-07-16T09:38:57Z","cross_cats_sorted":[],"title_canon_sha256":"c0c66b8359df8437bb4737b7c2ce0313c5b04025aae76b9512eebf8adf815ccd","abstract_canon_sha256":"02693aa497adb18fa0118b87f9724e7df1672734dc66859deba28d95a95908e9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:48:49.704273Z","signature_b64":"hp5QDgXrz3F3oOPVMNw4OssQZkdoIRr+rlvETzP1VHJl/P65LtivjTj/MmdZqRuvXrWObj+8RHKY7PXWQyOiBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6bd30848e7cec319788a8f92ea4849fb456dbca2acddf46b7b22c9b269a77606","last_reissued_at":"2026-05-18T01:48:49.703565Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:48:49.703565Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Bayesian Asteroseismology of 23 Solar-Like Kepler Targets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"David B. Guenther, Kieran MacLeod, Michael Gruberbauer, Thomas Kallinger","submitted_at":"2013-07-16T09:38:57Z","abstract_excerpt":"We study 23 previously published Kepler targets to perform a consistent grid-based Bayesian asteroseismic analysis and compare our results to those obtained via the Asteroseismic Modelling Portal (AMP). We find differences in the derived stellar parameters of many targets and their uncertainties. While some of these differences can be attributed to systematic effects between stellar evolutionary models, we show that the different methodologies deliver incompatible uncertainties for some parameters. Using non-adiabatic models and our capability to measure surface effects, we also investigate th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.4218","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":"1307.4218","created_at":"2026-05-18T01:48:49.703682+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.4218v1","created_at":"2026-05-18T01:48:49.703682+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.4218","created_at":"2026-05-18T01:48:49.703682+00:00"},{"alias_kind":"pith_short_12","alias_value":"NPJQQSHHZ3BR","created_at":"2026-05-18T12:27:52.871228+00:00"},{"alias_kind":"pith_short_16","alias_value":"NPJQQSHHZ3BRS6EK","created_at":"2026-05-18T12:27:52.871228+00:00"},{"alias_kind":"pith_short_8","alias_value":"NPJQQSHH","created_at":"2026-05-18T12:27:52.871228+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":221,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NPJQQSHHZ3BRS6EKR6JOUSCJ7N","json":"https://pith.science/pith/NPJQQSHHZ3BRS6EKR6JOUSCJ7N.json","graph_json":"https://pith.science/api/pith-number/NPJQQSHHZ3BRS6EKR6JOUSCJ7N/graph.json","events_json":"https://pith.science/api/pith-number/NPJQQSHHZ3BRS6EKR6JOUSCJ7N/events.json","paper":"https://pith.science/paper/NPJQQSHH"},"agent_actions":{"view_html":"https://pith.science/pith/NPJQQSHHZ3BRS6EKR6JOUSCJ7N","download_json":"https://pith.science/pith/NPJQQSHHZ3BRS6EKR6JOUSCJ7N.json","view_paper":"https://pith.science/paper/NPJQQSHH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.4218&json=true","fetch_graph":"https://pith.science/api/pith-number/NPJQQSHHZ3BRS6EKR6JOUSCJ7N/graph.json","fetch_events":"https://pith.science/api/pith-number/NPJQQSHHZ3BRS6EKR6JOUSCJ7N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NPJQQSHHZ3BRS6EKR6JOUSCJ7N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NPJQQSHHZ3BRS6EKR6JOUSCJ7N/action/storage_attestation","attest_author":"https://pith.science/pith/NPJQQSHHZ3BRS6EKR6JOUSCJ7N/action/author_attestation","sign_citation":"https://pith.science/pith/NPJQQSHHZ3BRS6EKR6JOUSCJ7N/action/citation_signature","submit_replication":"https://pith.science/pith/NPJQQSHHZ3BRS6EKR6JOUSCJ7N/action/replication_record"}},"created_at":"2026-05-18T01:48:49.703682+00:00","updated_at":"2026-05-18T01:48:49.703682+00:00"}