{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:FEVUZ6WYLSHXBZOFXZVMNOUBLT","short_pith_number":"pith:FEVUZ6WY","schema_version":"1.0","canonical_sha256":"292b4cfad85c8f70e5c5be6ac6ba815ccc9c0e93537ddf4b5f51f16ef88d5c76","source":{"kind":"arxiv","id":"1107.4008","version":1},"attestation_state":"computed","paper":{"title":"The Optical Gravitational Lensing Experiment. OGLE-III Photometric Maps of the Galactic Bulge Fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"1), 2), (2) Universidad de Concepci\\'on, (3) Institute of Astronomy, A. Udalski (1), Departamento de Astronomia, G. Pietrzy\\'nski (1, I. Soszy\\'nski (1), K. Ulaczyk (1) ((1) Warsaw University Observatory, {\\L}. Wyrzykowski (3, M. K. Szyma\\'nski (1), M. Kubiak (1), R. Poleski (1), University of Cambridge)","submitted_at":"2011-07-20T15:45:27Z","abstract_excerpt":"We present OGLE-III Photometric Maps of the Galactic bulge fields observed during the third phase of the OGLE project. This paper describes the last, concluding set of maps based on OGLE-III data.\n  The maps contain precise, calibrated VI photometry of about 340 million stars from 267 fields in the Galactic bulge observed during entire OGLE-III phase (2002-2009), covering about 92 square degrees in the sky. Precise astrometry of these objects is also provided.\n  We briefly discuss the photometry procedures and the quality of the data. We also present sample data and color-magnitude diagrams of"},"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":"1107.4008","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-07-20T15:45:27Z","cross_cats_sorted":[],"title_canon_sha256":"b01a2ce194ead6090a0a1cb729786e8eec73ca793f6b021a79069549c5618ec6","abstract_canon_sha256":"8de8c870f4ab5b2f68081acabacb65034627bce1f458a8177325a956da490333"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:17:14.227847Z","signature_b64":"XoubBMujAhD19eKaeORTOIXcGTvXpgDUow/75ZlmEBcgvlEaKqddbAc8s/GRGXi+hz+hygcisQ1cuwT5U7lRCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"292b4cfad85c8f70e5c5be6ac6ba815ccc9c0e93537ddf4b5f51f16ef88d5c76","last_reissued_at":"2026-05-18T04:17:14.227046Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:17:14.227046Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Optical Gravitational Lensing Experiment. OGLE-III Photometric Maps of the Galactic Bulge Fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"1), 2), (2) Universidad de Concepci\\'on, (3) Institute of Astronomy, A. Udalski (1), Departamento de Astronomia, G. Pietrzy\\'nski (1, I. Soszy\\'nski (1), K. Ulaczyk (1) ((1) Warsaw University Observatory, {\\L}. Wyrzykowski (3, M. K. Szyma\\'nski (1), M. Kubiak (1), R. Poleski (1), University of Cambridge)","submitted_at":"2011-07-20T15:45:27Z","abstract_excerpt":"We present OGLE-III Photometric Maps of the Galactic bulge fields observed during the third phase of the OGLE project. This paper describes the last, concluding set of maps based on OGLE-III data.\n  The maps contain precise, calibrated VI photometry of about 340 million stars from 267 fields in the Galactic bulge observed during entire OGLE-III phase (2002-2009), covering about 92 square degrees in the sky. Precise astrometry of these objects is also provided.\n  We briefly discuss the photometry procedures and the quality of the data. We also present sample data and color-magnitude diagrams of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1107.4008","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":"1107.4008","created_at":"2026-05-18T04:17:14.227175+00:00"},{"alias_kind":"arxiv_version","alias_value":"1107.4008v1","created_at":"2026-05-18T04:17:14.227175+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1107.4008","created_at":"2026-05-18T04:17:14.227175+00:00"},{"alias_kind":"pith_short_12","alias_value":"FEVUZ6WYLSHX","created_at":"2026-05-18T12:26:28.662955+00:00"},{"alias_kind":"pith_short_16","alias_value":"FEVUZ6WYLSHXBZOF","created_at":"2026-05-18T12:26:28.662955+00:00"},{"alias_kind":"pith_short_8","alias_value":"FEVUZ6WY","created_at":"2026-05-18T12:26:28.662955+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.08340","citing_title":"You Shall Not Pass (Without Modeling): High-Resolution Analysis of KMT-2019-BLG-0253 using MORIA","ref_index":30,"is_internal_anchor":false},{"citing_arxiv_id":"2605.06778","citing_title":"An HST Wide Field Survey of the Galactic Bulge: Overview, Strategy, and First Results","ref_index":285,"is_internal_anchor":false},{"citing_arxiv_id":"2605.06778","citing_title":"An HST Wide Field Survey of the Galactic Bulge: Overview, Strategy, and First Results","ref_index":103,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FEVUZ6WYLSHXBZOFXZVMNOUBLT","json":"https://pith.science/pith/FEVUZ6WYLSHXBZOFXZVMNOUBLT.json","graph_json":"https://pith.science/api/pith-number/FEVUZ6WYLSHXBZOFXZVMNOUBLT/graph.json","events_json":"https://pith.science/api/pith-number/FEVUZ6WYLSHXBZOFXZVMNOUBLT/events.json","paper":"https://pith.science/paper/FEVUZ6WY"},"agent_actions":{"view_html":"https://pith.science/pith/FEVUZ6WYLSHXBZOFXZVMNOUBLT","download_json":"https://pith.science/pith/FEVUZ6WYLSHXBZOFXZVMNOUBLT.json","view_paper":"https://pith.science/paper/FEVUZ6WY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1107.4008&json=true","fetch_graph":"https://pith.science/api/pith-number/FEVUZ6WYLSHXBZOFXZVMNOUBLT/graph.json","fetch_events":"https://pith.science/api/pith-number/FEVUZ6WYLSHXBZOFXZVMNOUBLT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FEVUZ6WYLSHXBZOFXZVMNOUBLT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FEVUZ6WYLSHXBZOFXZVMNOUBLT/action/storage_attestation","attest_author":"https://pith.science/pith/FEVUZ6WYLSHXBZOFXZVMNOUBLT/action/author_attestation","sign_citation":"https://pith.science/pith/FEVUZ6WYLSHXBZOFXZVMNOUBLT/action/citation_signature","submit_replication":"https://pith.science/pith/FEVUZ6WYLSHXBZOFXZVMNOUBLT/action/replication_record"}},"created_at":"2026-05-18T04:17:14.227175+00:00","updated_at":"2026-05-18T04:17:14.227175+00:00"}