{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:57PLY4GPAKIKFU6ZYCVSYVHYHT","short_pith_number":"pith:57PLY4GP","schema_version":"1.0","canonical_sha256":"efdebc70cf0290a2d3d9c0ab2c54f83ce53bb35e48b1e9fefa2c2e39030d43e8","source":{"kind":"arxiv","id":"1301.0023","version":1},"attestation_state":"computed","paper":{"title":"Characterizing the Cool KOIs IV: Kepler-32 as a prototype for the formation of compact planetary systems throughout the Galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Benjamin T. Montet, Daniel C. Fabrycky, John Asher Johnson, Jonathan J. Swift, Justin R. Crepp, Philip S. Muirhead, Timothy D. Morton","submitted_at":"2012-12-31T22:10:43Z","abstract_excerpt":"The Kepler space telescope has opened new vistas in exoplanet discovery space by revealing populations of Earth-sized planets that provide a new context for understanding planet formation. Approximately 70% of all stars in the Galaxy belong to the diminutive M dwarf class, several thousand of which lie within Kepler's field of view, and a large number of these targets show planet transit signals. Kepler-32 is a typical star in the Kepler M dwarf sample that presents us with a rare opportunity: five planets transit this star giving us an expansive view of its architecture. All five planets of t"},"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":"1301.0023","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2012-12-31T22:10:43Z","cross_cats_sorted":[],"title_canon_sha256":"1a9c321423d9fed0be41846b295d4eda8d99a744903521c668d199e8ab3cdfb5","abstract_canon_sha256":"55531665c3e2d13fa9152ad1e37fc5e5c94a00a75e342a976934d740a929706c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:52:22.484551Z","signature_b64":"uUMpCRA+4p2uEi3azDmSpTtf680eXjXoYR2yHWLeA8cmHvprldsD9gerMONKKRhN0cNSb6SvG6WuSRH1sdvcDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"efdebc70cf0290a2d3d9c0ab2c54f83ce53bb35e48b1e9fefa2c2e39030d43e8","last_reissued_at":"2026-05-18T01:52:22.483958Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:52:22.483958Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Characterizing the Cool KOIs IV: Kepler-32 as a prototype for the formation of compact planetary systems throughout the Galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Benjamin T. Montet, Daniel C. Fabrycky, John Asher Johnson, Jonathan J. Swift, Justin R. Crepp, Philip S. Muirhead, Timothy D. Morton","submitted_at":"2012-12-31T22:10:43Z","abstract_excerpt":"The Kepler space telescope has opened new vistas in exoplanet discovery space by revealing populations of Earth-sized planets that provide a new context for understanding planet formation. Approximately 70% of all stars in the Galaxy belong to the diminutive M dwarf class, several thousand of which lie within Kepler's field of view, and a large number of these targets show planet transit signals. Kepler-32 is a typical star in the Kepler M dwarf sample that presents us with a rare opportunity: five planets transit this star giving us an expansive view of its architecture. All five planets of t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.0023","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":"1301.0023","created_at":"2026-05-18T01:52:22.484045+00:00"},{"alias_kind":"arxiv_version","alias_value":"1301.0023v1","created_at":"2026-05-18T01:52:22.484045+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.0023","created_at":"2026-05-18T01:52:22.484045+00:00"},{"alias_kind":"pith_short_12","alias_value":"57PLY4GPAKIK","created_at":"2026-05-18T12:26:53.410803+00:00"},{"alias_kind":"pith_short_16","alias_value":"57PLY4GPAKIKFU6Z","created_at":"2026-05-18T12:26:53.410803+00:00"},{"alias_kind":"pith_short_8","alias_value":"57PLY4GP","created_at":"2026-05-18T12:26:53.410803+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/57PLY4GPAKIKFU6ZYCVSYVHYHT","json":"https://pith.science/pith/57PLY4GPAKIKFU6ZYCVSYVHYHT.json","graph_json":"https://pith.science/api/pith-number/57PLY4GPAKIKFU6ZYCVSYVHYHT/graph.json","events_json":"https://pith.science/api/pith-number/57PLY4GPAKIKFU6ZYCVSYVHYHT/events.json","paper":"https://pith.science/paper/57PLY4GP"},"agent_actions":{"view_html":"https://pith.science/pith/57PLY4GPAKIKFU6ZYCVSYVHYHT","download_json":"https://pith.science/pith/57PLY4GPAKIKFU6ZYCVSYVHYHT.json","view_paper":"https://pith.science/paper/57PLY4GP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1301.0023&json=true","fetch_graph":"https://pith.science/api/pith-number/57PLY4GPAKIKFU6ZYCVSYVHYHT/graph.json","fetch_events":"https://pith.science/api/pith-number/57PLY4GPAKIKFU6ZYCVSYVHYHT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/57PLY4GPAKIKFU6ZYCVSYVHYHT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/57PLY4GPAKIKFU6ZYCVSYVHYHT/action/storage_attestation","attest_author":"https://pith.science/pith/57PLY4GPAKIKFU6ZYCVSYVHYHT/action/author_attestation","sign_citation":"https://pith.science/pith/57PLY4GPAKIKFU6ZYCVSYVHYHT/action/citation_signature","submit_replication":"https://pith.science/pith/57PLY4GPAKIKFU6ZYCVSYVHYHT/action/replication_record"}},"created_at":"2026-05-18T01:52:22.484045+00:00","updated_at":"2026-05-18T01:52:22.484045+00:00"}