{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:HKUSLR3HEZNAZB3THCPLMJTRZN","short_pith_number":"pith:HKUSLR3H","schema_version":"1.0","canonical_sha256":"3aa925c767265a0c8773389eb62671cb4592f8457ef31574e006e5d6ba3e2a16","source":{"kind":"arxiv","id":"1909.11927","version":2},"attestation_state":"computed","paper":{"title":"The Bayesian Asteroseismology data Modeling pipeline and its application to $\\it K2$ data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Daniel Huber, Dennis Stello, Joel C. Zinn, Sanjib Sharma","submitted_at":"2019-09-26T06:27:19Z","abstract_excerpt":"We present the Bayesian Asteroseismology data Modeling (BAM) pipeline, an automated asteroseismology pipeline that returns global oscillation parameters and granulation parameters from the analysis of photometric time-series. BAM also determines if a star is likely to be a solar-like oscillator. We have designed BAM to specially process ${\\it K2}$ light curves, which suffer from unique noise signatures that can confuse asteroseismic analysis, though it may be used on any photometric time series --- including those from ${\\it Kepler}$ and ${\\it TESS}$. We demonstrate the BAM oscillation paramet"},"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":"1909.11927","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2019-09-26T06:27:19Z","cross_cats_sorted":[],"title_canon_sha256":"57e68a6ff0e2a649d6800777e3ecdf5a3e6f99de6fdf47926487c7516e0a82b2","abstract_canon_sha256":"ba409d71d8acf49253e148979642a331f32a02762b329bf864dd78daa2c66ac0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:20:32.023929Z","signature_b64":"CTHg1nK/lXwtujKFjwOk+QQud0zFb+bvvstXeJUoFJ6xorqOLPi3RlJnkx54FxVjaK5aAnK5TY9sNf+TpqkjBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3aa925c767265a0c8773389eb62671cb4592f8457ef31574e006e5d6ba3e2a16","last_reissued_at":"2026-07-05T00:20:32.023536Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:20:32.023536Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Bayesian Asteroseismology data Modeling pipeline and its application to $\\it K2$ data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Daniel Huber, Dennis Stello, Joel C. Zinn, Sanjib Sharma","submitted_at":"2019-09-26T06:27:19Z","abstract_excerpt":"We present the Bayesian Asteroseismology data Modeling (BAM) pipeline, an automated asteroseismology pipeline that returns global oscillation parameters and granulation parameters from the analysis of photometric time-series. BAM also determines if a star is likely to be a solar-like oscillator. We have designed BAM to specially process ${\\it K2}$ light curves, which suffer from unique noise signatures that can confuse asteroseismic analysis, though it may be used on any photometric time series --- including those from ${\\it Kepler}$ and ${\\it TESS}$. We demonstrate the BAM oscillation paramet"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1909.11927","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1909.11927/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"1909.11927","created_at":"2026-07-05T00:20:32.023592+00:00"},{"alias_kind":"arxiv_version","alias_value":"1909.11927v2","created_at":"2026-07-05T00:20:32.023592+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1909.11927","created_at":"2026-07-05T00:20:32.023592+00:00"},{"alias_kind":"pith_short_12","alias_value":"HKUSLR3HEZNA","created_at":"2026-07-05T00:20:32.023592+00:00"},{"alias_kind":"pith_short_16","alias_value":"HKUSLR3HEZNAZB3T","created_at":"2026-07-05T00:20:32.023592+00:00"},{"alias_kind":"pith_short_8","alias_value":"HKUSLR3H","created_at":"2026-07-05T00:20:32.023592+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/HKUSLR3HEZNAZB3THCPLMJTRZN","json":"https://pith.science/pith/HKUSLR3HEZNAZB3THCPLMJTRZN.json","graph_json":"https://pith.science/api/pith-number/HKUSLR3HEZNAZB3THCPLMJTRZN/graph.json","events_json":"https://pith.science/api/pith-number/HKUSLR3HEZNAZB3THCPLMJTRZN/events.json","paper":"https://pith.science/paper/HKUSLR3H"},"agent_actions":{"view_html":"https://pith.science/pith/HKUSLR3HEZNAZB3THCPLMJTRZN","download_json":"https://pith.science/pith/HKUSLR3HEZNAZB3THCPLMJTRZN.json","view_paper":"https://pith.science/paper/HKUSLR3H","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1909.11927&json=true","fetch_graph":"https://pith.science/api/pith-number/HKUSLR3HEZNAZB3THCPLMJTRZN/graph.json","fetch_events":"https://pith.science/api/pith-number/HKUSLR3HEZNAZB3THCPLMJTRZN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HKUSLR3HEZNAZB3THCPLMJTRZN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HKUSLR3HEZNAZB3THCPLMJTRZN/action/storage_attestation","attest_author":"https://pith.science/pith/HKUSLR3HEZNAZB3THCPLMJTRZN/action/author_attestation","sign_citation":"https://pith.science/pith/HKUSLR3HEZNAZB3THCPLMJTRZN/action/citation_signature","submit_replication":"https://pith.science/pith/HKUSLR3HEZNAZB3THCPLMJTRZN/action/replication_record"}},"created_at":"2026-07-05T00:20:32.023592+00:00","updated_at":"2026-07-05T00:20:32.023592+00:00"}