{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:PQGVH7VZSQ57CHTJQ3J4MD22IP","short_pith_number":"pith:PQGVH7VZ","schema_version":"1.0","canonical_sha256":"7c0d53feb9943bf11e6986d3c60f5a43c63fe1d26fe5619180a63619693aef1f","source":{"kind":"arxiv","id":"2001.07737","version":3},"attestation_state":"computed","paper":{"title":"The Gaia-Kepler Stellar Properties Catalog. I. Homogeneous Fundamental Properties for 186,301 Kepler Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Adam L. Kraus, Daniel Huber, Eric Gaidos, Jamie Tayar, Jennifer L. van Saders, Travis A. Berger","submitted_at":"2020-01-21T19:05:51Z","abstract_excerpt":"An accurate and precise Kepler Stellar Properties Catalog is essential for the interpretation of the Kepler exoplanet survey results. Previous Kepler Stellar Properties Catalogs have focused on reporting the best-available parameters for each star, but this has required combining data from a variety of heterogeneous sources. We present the Gaia-Kepler Stellar Properties Catalog, a set of stellar properties of 186,301 Kepler stars, homogeneously derived from isochrones and broadband photometry, Gaia Data Release 2 parallaxes, and spectroscopic metallicities, where available. Our photometric eff"},"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":"2001.07737","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2020-01-21T19:05:51Z","cross_cats_sorted":["astro-ph.EP","astro-ph.GA"],"title_canon_sha256":"3fea812c342cea04103fd3c8fb430e40fb4fc8258168f76a6e5f3d97d15df0e5","abstract_canon_sha256":"3112cf1da5c1dc6b8ab087a55c88d17d51641aa4e517acda9db8770a5951ef7f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:07:39.563906Z","signature_b64":"ONWb0jvHioZqjYMxAFNAKUj4T2nnWzMtrRvDMho0Fm2aWBRxSWmqnhYeslBt+7dZV0rhSAZtX9WIt4CHTI/lBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7c0d53feb9943bf11e6986d3c60f5a43c63fe1d26fe5619180a63619693aef1f","last_reissued_at":"2026-07-05T01:07:39.563357Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:07:39.563357Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Gaia-Kepler Stellar Properties Catalog. I. Homogeneous Fundamental Properties for 186,301 Kepler Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Adam L. Kraus, Daniel Huber, Eric Gaidos, Jamie Tayar, Jennifer L. van Saders, Travis A. Berger","submitted_at":"2020-01-21T19:05:51Z","abstract_excerpt":"An accurate and precise Kepler Stellar Properties Catalog is essential for the interpretation of the Kepler exoplanet survey results. Previous Kepler Stellar Properties Catalogs have focused on reporting the best-available parameters for each star, but this has required combining data from a variety of heterogeneous sources. We present the Gaia-Kepler Stellar Properties Catalog, a set of stellar properties of 186,301 Kepler stars, homogeneously derived from isochrones and broadband photometry, Gaia Data Release 2 parallaxes, and spectroscopic metallicities, where available. Our photometric eff"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2001.07737","kind":"arxiv","version":3},"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/2001.07737/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":"2001.07737","created_at":"2026-07-05T01:07:39.563415+00:00"},{"alias_kind":"arxiv_version","alias_value":"2001.07737v3","created_at":"2026-07-05T01:07:39.563415+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2001.07737","created_at":"2026-07-05T01:07:39.563415+00:00"},{"alias_kind":"pith_short_12","alias_value":"PQGVH7VZSQ57","created_at":"2026-07-05T01:07:39.563415+00:00"},{"alias_kind":"pith_short_16","alias_value":"PQGVH7VZSQ57CHTJ","created_at":"2026-07-05T01:07:39.563415+00:00"},{"alias_kind":"pith_short_8","alias_value":"PQGVH7VZ","created_at":"2026-07-05T01:07:39.563415+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06708","citing_title":"Mitigating Charge Migration in JWST NIRISS Reveals That KELT-7 b is a Metal-enriched Ultra-hot Jupiter Orbiting a Young Metal-rich Star","ref_index":208,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PQGVH7VZSQ57CHTJQ3J4MD22IP","json":"https://pith.science/pith/PQGVH7VZSQ57CHTJQ3J4MD22IP.json","graph_json":"https://pith.science/api/pith-number/PQGVH7VZSQ57CHTJQ3J4MD22IP/graph.json","events_json":"https://pith.science/api/pith-number/PQGVH7VZSQ57CHTJQ3J4MD22IP/events.json","paper":"https://pith.science/paper/PQGVH7VZ"},"agent_actions":{"view_html":"https://pith.science/pith/PQGVH7VZSQ57CHTJQ3J4MD22IP","download_json":"https://pith.science/pith/PQGVH7VZSQ57CHTJQ3J4MD22IP.json","view_paper":"https://pith.science/paper/PQGVH7VZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2001.07737&json=true","fetch_graph":"https://pith.science/api/pith-number/PQGVH7VZSQ57CHTJQ3J4MD22IP/graph.json","fetch_events":"https://pith.science/api/pith-number/PQGVH7VZSQ57CHTJQ3J4MD22IP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PQGVH7VZSQ57CHTJQ3J4MD22IP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PQGVH7VZSQ57CHTJQ3J4MD22IP/action/storage_attestation","attest_author":"https://pith.science/pith/PQGVH7VZSQ57CHTJQ3J4MD22IP/action/author_attestation","sign_citation":"https://pith.science/pith/PQGVH7VZSQ57CHTJQ3J4MD22IP/action/citation_signature","submit_replication":"https://pith.science/pith/PQGVH7VZSQ57CHTJQ3J4MD22IP/action/replication_record"}},"created_at":"2026-07-05T01:07:39.563415+00:00","updated_at":"2026-07-05T01:07:39.563415+00:00"}