{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:CSFH2FHQARKNG7V5Z37T3P4A3X","short_pith_number":"pith:CSFH2FHQ","schema_version":"1.0","canonical_sha256":"148a7d14f00454d37ebdceff3dbf80ddc07e7f181d1b9e359fbaf1778377e4e1","source":{"kind":"arxiv","id":"1109.2063","version":1},"attestation_state":"computed","paper":{"title":"Accurate Low-Mass Stellar Models of KOI-126","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Aaron Dotter, Brian Chaboyer, Gregory A. Feiden","submitted_at":"2011-09-09T16:38:42Z","abstract_excerpt":"The recent discovery of an eclipsing hierarchical triple system with two low-mass stars in a close orbit (KOI-126) by Carter et al. (2011) appeared to reinforce the evidence that theoretical stellar evolution models are not able to reproduce the observational mass-radius relation for low-mass stars. We present a set of stellar models for the three stars in the KOI-126 system that show excellent agreement with the observed radii. This agreement appears to be due to the equation of state implemented by our code. A significant dispersion in the observed mass-radius relation for fully convective s"},"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":"1109.2063","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-09-09T16:38:42Z","cross_cats_sorted":[],"title_canon_sha256":"6cf08b252a6be8d2564eb52e7fae8b6e109bc049dcf21976b15967b033a1c1d4","abstract_canon_sha256":"9a15564657537cc9f1798f3613c6656f8766eba29b3fe449541212e36d599e69"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:51:23.778995Z","signature_b64":"K7axLju62qz3eNbYVO9oG2j2cLuyHMDTtRgUE0ZwQSXYKY4jIUznDUcgHxQW1adtU5Cn0qne4va5/tigjsF7BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"148a7d14f00454d37ebdceff3dbf80ddc07e7f181d1b9e359fbaf1778377e4e1","last_reissued_at":"2026-05-18T03:51:23.778133Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:51:23.778133Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Accurate Low-Mass Stellar Models of KOI-126","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Aaron Dotter, Brian Chaboyer, Gregory A. Feiden","submitted_at":"2011-09-09T16:38:42Z","abstract_excerpt":"The recent discovery of an eclipsing hierarchical triple system with two low-mass stars in a close orbit (KOI-126) by Carter et al. (2011) appeared to reinforce the evidence that theoretical stellar evolution models are not able to reproduce the observational mass-radius relation for low-mass stars. We present a set of stellar models for the three stars in the KOI-126 system that show excellent agreement with the observed radii. This agreement appears to be due to the equation of state implemented by our code. A significant dispersion in the observed mass-radius relation for fully convective s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1109.2063","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":"1109.2063","created_at":"2026-05-18T03:51:23.778290+00:00"},{"alias_kind":"arxiv_version","alias_value":"1109.2063v1","created_at":"2026-05-18T03:51:23.778290+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1109.2063","created_at":"2026-05-18T03:51:23.778290+00:00"},{"alias_kind":"pith_short_12","alias_value":"CSFH2FHQARKN","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_16","alias_value":"CSFH2FHQARKNG7V5","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_8","alias_value":"CSFH2FHQ","created_at":"2026-05-18T12:26:26.731475+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/CSFH2FHQARKNG7V5Z37T3P4A3X","json":"https://pith.science/pith/CSFH2FHQARKNG7V5Z37T3P4A3X.json","graph_json":"https://pith.science/api/pith-number/CSFH2FHQARKNG7V5Z37T3P4A3X/graph.json","events_json":"https://pith.science/api/pith-number/CSFH2FHQARKNG7V5Z37T3P4A3X/events.json","paper":"https://pith.science/paper/CSFH2FHQ"},"agent_actions":{"view_html":"https://pith.science/pith/CSFH2FHQARKNG7V5Z37T3P4A3X","download_json":"https://pith.science/pith/CSFH2FHQARKNG7V5Z37T3P4A3X.json","view_paper":"https://pith.science/paper/CSFH2FHQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1109.2063&json=true","fetch_graph":"https://pith.science/api/pith-number/CSFH2FHQARKNG7V5Z37T3P4A3X/graph.json","fetch_events":"https://pith.science/api/pith-number/CSFH2FHQARKNG7V5Z37T3P4A3X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CSFH2FHQARKNG7V5Z37T3P4A3X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CSFH2FHQARKNG7V5Z37T3P4A3X/action/storage_attestation","attest_author":"https://pith.science/pith/CSFH2FHQARKNG7V5Z37T3P4A3X/action/author_attestation","sign_citation":"https://pith.science/pith/CSFH2FHQARKNG7V5Z37T3P4A3X/action/citation_signature","submit_replication":"https://pith.science/pith/CSFH2FHQARKNG7V5Z37T3P4A3X/action/replication_record"}},"created_at":"2026-05-18T03:51:23.778290+00:00","updated_at":"2026-05-18T03:51:23.778290+00:00"}