{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:733UEXGQL4BDGTNVDFEUQT3LS2","short_pith_number":"pith:733UEXGQ","schema_version":"1.0","canonical_sha256":"fef7425cd05f02334db51949484f6b96b0737ff8269fc4ebec50010c40a56a34","source":{"kind":"arxiv","id":"1403.6045","version":1},"attestation_state":"computed","paper":{"title":"Gaia photometry for white dwarfs","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"A.C. Robin, C. Jordi, J.M. Carrasco, P.E. Tremblay, P.M Kowalski, R. Napiwotzki, S. Catal\\'an, X. Luri","submitted_at":"2014-03-24T17:07:49Z","abstract_excerpt":"Context. White dwarfs can be used to study the structure and evolution of the Galaxy by analysing their luminosity function and initial mass function. Among them, the very cool white dwarfs provide the information for the early ages of each population. Because white dwarfs are intrinsically faint only the nearby (about 20 pc) sample is reasonably complete. The Gaia space mission will drastically increase the sample of known white dwarfs through its 5-6 years survey of the whole sky up to magnitude V = 20-25.\n  Aims. We provide a characterisation of Gaia photometry for white dwarfs to better pr"},"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":"1403.6045","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","primary_cat":"astro-ph.IM","submitted_at":"2014-03-24T17:07:49Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"72a4ec4207dfa1597213d4b47af7b295333eb53c5db665922d16d41d0f4e4917","abstract_canon_sha256":"9802dc5d7b55badf7e02600b417da146e2dc47108c52a03c691339b6ff63feab"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:52:25.263506Z","signature_b64":"VUv/dVspq6FQZEriIGTN8cRq0+mhiNQHNbx1k0T8A4icV3xQQ6mfwmnYh5ACZRWIFDkTYatKKPDfxswddeTOCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fef7425cd05f02334db51949484f6b96b0737ff8269fc4ebec50010c40a56a34","last_reissued_at":"2026-05-18T02:52:25.262728Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:52:25.262728Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gaia photometry for white dwarfs","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"A.C. Robin, C. Jordi, J.M. Carrasco, P.E. Tremblay, P.M Kowalski, R. Napiwotzki, S. Catal\\'an, X. Luri","submitted_at":"2014-03-24T17:07:49Z","abstract_excerpt":"Context. White dwarfs can be used to study the structure and evolution of the Galaxy by analysing their luminosity function and initial mass function. Among them, the very cool white dwarfs provide the information for the early ages of each population. Because white dwarfs are intrinsically faint only the nearby (about 20 pc) sample is reasonably complete. The Gaia space mission will drastically increase the sample of known white dwarfs through its 5-6 years survey of the whole sky up to magnitude V = 20-25.\n  Aims. We provide a characterisation of Gaia photometry for white dwarfs to better pr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.6045","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":"1403.6045","created_at":"2026-05-18T02:52:25.262820+00:00"},{"alias_kind":"arxiv_version","alias_value":"1403.6045v1","created_at":"2026-05-18T02:52:25.262820+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.6045","created_at":"2026-05-18T02:52:25.262820+00:00"},{"alias_kind":"pith_short_12","alias_value":"733UEXGQL4BD","created_at":"2026-05-18T12:28:16.859392+00:00"},{"alias_kind":"pith_short_16","alias_value":"733UEXGQL4BDGTNV","created_at":"2026-05-18T12:28:16.859392+00:00"},{"alias_kind":"pith_short_8","alias_value":"733UEXGQ","created_at":"2026-05-18T12:28:16.859392+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/733UEXGQL4BDGTNVDFEUQT3LS2","json":"https://pith.science/pith/733UEXGQL4BDGTNVDFEUQT3LS2.json","graph_json":"https://pith.science/api/pith-number/733UEXGQL4BDGTNVDFEUQT3LS2/graph.json","events_json":"https://pith.science/api/pith-number/733UEXGQL4BDGTNVDFEUQT3LS2/events.json","paper":"https://pith.science/paper/733UEXGQ"},"agent_actions":{"view_html":"https://pith.science/pith/733UEXGQL4BDGTNVDFEUQT3LS2","download_json":"https://pith.science/pith/733UEXGQL4BDGTNVDFEUQT3LS2.json","view_paper":"https://pith.science/paper/733UEXGQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1403.6045&json=true","fetch_graph":"https://pith.science/api/pith-number/733UEXGQL4BDGTNVDFEUQT3LS2/graph.json","fetch_events":"https://pith.science/api/pith-number/733UEXGQL4BDGTNVDFEUQT3LS2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/733UEXGQL4BDGTNVDFEUQT3LS2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/733UEXGQL4BDGTNVDFEUQT3LS2/action/storage_attestation","attest_author":"https://pith.science/pith/733UEXGQL4BDGTNVDFEUQT3LS2/action/author_attestation","sign_citation":"https://pith.science/pith/733UEXGQL4BDGTNVDFEUQT3LS2/action/citation_signature","submit_replication":"https://pith.science/pith/733UEXGQL4BDGTNVDFEUQT3LS2/action/replication_record"}},"created_at":"2026-05-18T02:52:25.262820+00:00","updated_at":"2026-05-18T02:52:25.262820+00:00"}