{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:4M3B4EOAQQ6ATS3KVRSUHTUF7B","short_pith_number":"pith:4M3B4EOA","schema_version":"1.0","canonical_sha256":"e3361e11c0843c09cb6aac6543ce85f876f491cdb9b3c4c9709566a32914331d","source":{"kind":"arxiv","id":"1805.11395","version":2},"attestation_state":"computed","paper":{"title":"Gaia Data Release 2: Validation of the classification of RR Lyrae and Cepheid variables with the Kepler and K2 missions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"\\'Aron L. Juh\\'asz, Emese Plachy, L\\'aszl\\'o Moln\\'ar, Lorenzo Rimoldini","submitted_at":"2018-05-29T12:38:44Z","abstract_excerpt":"The second data release of the Gaia mission includes an advance catalog of variable stars. The classification of these stars are based on sparse photometry from the first 22 months of the mission. We set out to investigate the purity and completeness of the all-sky Gaia classification results with the help of the continuous light curves of the observed targets from the Kepler and K2 missions, focusing specifically on RR Lyrae and Cepheid pulsators, outside the Galactic Bulge region. We crossmatched the Gaia identifications with the observations collected by the Kepler space telescope. We inspe"},"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":"1805.11395","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-05-29T12:38:44Z","cross_cats_sorted":[],"title_canon_sha256":"6a4003b7423a6d9ab57bca27e6146c19e89365ef238d61830d26de255ecbbc59","abstract_canon_sha256":"49e02cbb91ee2b92199d11f1a6ea9ecc36868a50a1bf1a61e4fc506b7dea78a2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:58:41.302670Z","signature_b64":"z6F8VQhZrldUN6h1z1WR0UE2Ox9OXPmfQnPqB8p4/Kbl/NYP6kwkMQhC2OoQ293RduD6uOOMgGT6iRR1wYtxAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e3361e11c0843c09cb6aac6543ce85f876f491cdb9b3c4c9709566a32914331d","last_reissued_at":"2026-05-17T23:58:41.301954Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:58:41.301954Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gaia Data Release 2: Validation of the classification of RR Lyrae and Cepheid variables with the Kepler and K2 missions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"\\'Aron L. Juh\\'asz, Emese Plachy, L\\'aszl\\'o Moln\\'ar, Lorenzo Rimoldini","submitted_at":"2018-05-29T12:38:44Z","abstract_excerpt":"The second data release of the Gaia mission includes an advance catalog of variable stars. The classification of these stars are based on sparse photometry from the first 22 months of the mission. We set out to investigate the purity and completeness of the all-sky Gaia classification results with the help of the continuous light curves of the observed targets from the Kepler and K2 missions, focusing specifically on RR Lyrae and Cepheid pulsators, outside the Galactic Bulge region. We crossmatched the Gaia identifications with the observations collected by the Kepler space telescope. We inspe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1805.11395","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":""},"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":"1805.11395","created_at":"2026-05-17T23:58:41.302075+00:00"},{"alias_kind":"arxiv_version","alias_value":"1805.11395v2","created_at":"2026-05-17T23:58:41.302075+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1805.11395","created_at":"2026-05-17T23:58:41.302075+00:00"},{"alias_kind":"pith_short_12","alias_value":"4M3B4EOAQQ6A","created_at":"2026-05-18T12:32:05.422762+00:00"},{"alias_kind":"pith_short_16","alias_value":"4M3B4EOAQQ6ATS3K","created_at":"2026-05-18T12:32:05.422762+00:00"},{"alias_kind":"pith_short_8","alias_value":"4M3B4EOA","created_at":"2026-05-18T12:32:05.422762+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/4M3B4EOAQQ6ATS3KVRSUHTUF7B","json":"https://pith.science/pith/4M3B4EOAQQ6ATS3KVRSUHTUF7B.json","graph_json":"https://pith.science/api/pith-number/4M3B4EOAQQ6ATS3KVRSUHTUF7B/graph.json","events_json":"https://pith.science/api/pith-number/4M3B4EOAQQ6ATS3KVRSUHTUF7B/events.json","paper":"https://pith.science/paper/4M3B4EOA"},"agent_actions":{"view_html":"https://pith.science/pith/4M3B4EOAQQ6ATS3KVRSUHTUF7B","download_json":"https://pith.science/pith/4M3B4EOAQQ6ATS3KVRSUHTUF7B.json","view_paper":"https://pith.science/paper/4M3B4EOA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1805.11395&json=true","fetch_graph":"https://pith.science/api/pith-number/4M3B4EOAQQ6ATS3KVRSUHTUF7B/graph.json","fetch_events":"https://pith.science/api/pith-number/4M3B4EOAQQ6ATS3KVRSUHTUF7B/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4M3B4EOAQQ6ATS3KVRSUHTUF7B/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4M3B4EOAQQ6ATS3KVRSUHTUF7B/action/storage_attestation","attest_author":"https://pith.science/pith/4M3B4EOAQQ6ATS3KVRSUHTUF7B/action/author_attestation","sign_citation":"https://pith.science/pith/4M3B4EOAQQ6ATS3KVRSUHTUF7B/action/citation_signature","submit_replication":"https://pith.science/pith/4M3B4EOAQQ6ATS3KVRSUHTUF7B/action/replication_record"}},"created_at":"2026-05-17T23:58:41.302075+00:00","updated_at":"2026-05-17T23:58:41.302075+00:00"}