{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:BMB7FSKJCUPPNIVYHJBSLOSFAP","short_pith_number":"pith:BMB7FSKJ","schema_version":"1.0","canonical_sha256":"0b03f2c949151ef6a2b83a4325ba4503e8c74c852e8feaa04d0831688e4c5bf8","source":{"kind":"arxiv","id":"astro-ph/0604234","version":1},"attestation_state":"computed","paper":{"title":"Two extremely metal-poor emission-line galaxies in the Sloan Digital Sky Survey","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) Institute for Astrophysics, (3) University of Virginia, Charlottesville, Germany, Goettingen, K. J. Fricke (2), Kyiv, N. G. Guseva (1), P. Papaderos (2), T. X. Thuan (3) ((1) Main Astronomical Observatory, Ukraine, USA), Y. I. Izotov (1)","submitted_at":"2006-04-11T09:15:25Z","abstract_excerpt":"We present spectroscopic observations with the 3.6m ESO telescope of two emission-line galaxies, J2104-0035 and J0113+0052, selected from the Data Release 4 (DR4) of the Sloan Digital Sky Survey (SDSS). From our data we determine the oxygen abundance of these systems to be respectively 12+logO/H = 7.26+/-0.03 and 7.17+/-0.09, making them the two most metal-deficient galaxies found thus far in the SDSS and placing them among the five most metal-deficient emission-line galaxies ever discovered. Their oxygen abundances are close to those of the two most metal-deficient emission-line galaxies know"},"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":"astro-ph/0604234","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-04-11T09:15:25Z","cross_cats_sorted":[],"title_canon_sha256":"45cc3b59122fca5da7dcc60f85dd4548dc0850bde5a74b93bef2b6c6d1c12de7","abstract_canon_sha256":"f23c29a1224581048dc6b6ee1d2ddee85901b7779cbda25c486ef45ee88be920"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:14:41.818066Z","signature_b64":"dZhvnnlMa9k6jl42q/aldTkndLwmX6CqCJOXVnHQhuJjnNSF4lAXQdO5k7U92vfqJ8JpWj34I5CME6TzIXiKCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0b03f2c949151ef6a2b83a4325ba4503e8c74c852e8feaa04d0831688e4c5bf8","last_reissued_at":"2026-05-18T00:14:41.817447Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:14:41.817447Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Two extremely metal-poor emission-line galaxies in the Sloan Digital Sky Survey","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) Institute for Astrophysics, (3) University of Virginia, Charlottesville, Germany, Goettingen, K. J. Fricke (2), Kyiv, N. G. Guseva (1), P. Papaderos (2), T. X. Thuan (3) ((1) Main Astronomical Observatory, Ukraine, USA), Y. I. Izotov (1)","submitted_at":"2006-04-11T09:15:25Z","abstract_excerpt":"We present spectroscopic observations with the 3.6m ESO telescope of two emission-line galaxies, J2104-0035 and J0113+0052, selected from the Data Release 4 (DR4) of the Sloan Digital Sky Survey (SDSS). From our data we determine the oxygen abundance of these systems to be respectively 12+logO/H = 7.26+/-0.03 and 7.17+/-0.09, making them the two most metal-deficient galaxies found thus far in the SDSS and placing them among the five most metal-deficient emission-line galaxies ever discovered. Their oxygen abundances are close to those of the two most metal-deficient emission-line galaxies know"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0604234","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":"astro-ph/0604234","created_at":"2026-05-18T00:14:41.817560+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0604234v1","created_at":"2026-05-18T00:14:41.817560+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0604234","created_at":"2026-05-18T00:14:41.817560+00:00"},{"alias_kind":"pith_short_12","alias_value":"BMB7FSKJCUPP","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_16","alias_value":"BMB7FSKJCUPPNIVY","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_8","alias_value":"BMB7FSKJ","created_at":"2026-05-18T12:25:53.939244+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/BMB7FSKJCUPPNIVYHJBSLOSFAP","json":"https://pith.science/pith/BMB7FSKJCUPPNIVYHJBSLOSFAP.json","graph_json":"https://pith.science/api/pith-number/BMB7FSKJCUPPNIVYHJBSLOSFAP/graph.json","events_json":"https://pith.science/api/pith-number/BMB7FSKJCUPPNIVYHJBSLOSFAP/events.json","paper":"https://pith.science/paper/BMB7FSKJ"},"agent_actions":{"view_html":"https://pith.science/pith/BMB7FSKJCUPPNIVYHJBSLOSFAP","download_json":"https://pith.science/pith/BMB7FSKJCUPPNIVYHJBSLOSFAP.json","view_paper":"https://pith.science/paper/BMB7FSKJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0604234&json=true","fetch_graph":"https://pith.science/api/pith-number/BMB7FSKJCUPPNIVYHJBSLOSFAP/graph.json","fetch_events":"https://pith.science/api/pith-number/BMB7FSKJCUPPNIVYHJBSLOSFAP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BMB7FSKJCUPPNIVYHJBSLOSFAP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BMB7FSKJCUPPNIVYHJBSLOSFAP/action/storage_attestation","attest_author":"https://pith.science/pith/BMB7FSKJCUPPNIVYHJBSLOSFAP/action/author_attestation","sign_citation":"https://pith.science/pith/BMB7FSKJCUPPNIVYHJBSLOSFAP/action/citation_signature","submit_replication":"https://pith.science/pith/BMB7FSKJCUPPNIVYHJBSLOSFAP/action/replication_record"}},"created_at":"2026-05-18T00:14:41.817560+00:00","updated_at":"2026-05-18T00:14:41.817560+00:00"}