{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:ZPDPLQANNHBMZ4J4R62NIUXALV","short_pith_number":"pith:ZPDPLQAN","schema_version":"1.0","canonical_sha256":"cbc6f5c00d69c2ccf13c8fb4d452e05d7a9828bcac604886c24ee38255d45adb","source":{"kind":"arxiv","id":"astro-ph/0409448","version":1},"attestation_state":"computed","paper":{"title":"Absorption Line Study of Halo Gas in NGC 3067 Toward the Background Quasar 3C 232","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) NAIC, (3) Nrao, (4) Univ. of Chicago), Arecibo, Brian A. Keeney (1), Chris L. Carilli (3), Emmanuel Momjian (2), Jason Tumlinson (4) ((1) CASA, John T. Stocke (1), Univ. of Colorado","submitted_at":"2004-09-17T22:04:59Z","abstract_excerpt":"We present new H I 21 cm absorption data and ultraviolet spectroscopy from HST/STIS of the QSO/galaxy pair 3C 232/NGC 3067. The QSO sightline lies near the minor axis and 1.8 arcmin (11 kpc) above the plane of NGC 3067, a nearby luminous (cz = 1465 km/s, L = 0.5L*) starburst galaxy with a moderate star formation rate of 1.4 Solar masses per year. The UV spectra show that the Si IV and C IV doublets have the same three velocity components at cz = 1369, 1417, and 1530 km/s found in Ca II H & K, Na I D, Mg I, Mg II, and Fe II, implying that the low and high ionization gas are both found in three "},"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/0409448","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2004-09-17T22:04:59Z","cross_cats_sorted":[],"title_canon_sha256":"fc00884763abf3d16e71ef2510eafbabf51bbcdc18bd2844d5b1b2a313f51a81","abstract_canon_sha256":"a6c36ea0fbf723124beb9897435983124ddd5f1fd27bc386c51c5108664de3f0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:44:43.128715Z","signature_b64":"5JBEk7AYDP3Qlk/8ATtFiyv+xV6/RqOYuBjbuNOnr+rFds1/ipPCaNoarNcQlxlm/u5NhOCXHNIZzA4TDActAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cbc6f5c00d69c2ccf13c8fb4d452e05d7a9828bcac604886c24ee38255d45adb","last_reissued_at":"2026-07-04T16:44:43.128361Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:44:43.128361Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Absorption Line Study of Halo Gas in NGC 3067 Toward the Background Quasar 3C 232","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) NAIC, (3) Nrao, (4) Univ. of Chicago), Arecibo, Brian A. Keeney (1), Chris L. Carilli (3), Emmanuel Momjian (2), Jason Tumlinson (4) ((1) CASA, John T. Stocke (1), Univ. of Colorado","submitted_at":"2004-09-17T22:04:59Z","abstract_excerpt":"We present new H I 21 cm absorption data and ultraviolet spectroscopy from HST/STIS of the QSO/galaxy pair 3C 232/NGC 3067. The QSO sightline lies near the minor axis and 1.8 arcmin (11 kpc) above the plane of NGC 3067, a nearby luminous (cz = 1465 km/s, L = 0.5L*) starburst galaxy with a moderate star formation rate of 1.4 Solar masses per year. The UV spectra show that the Si IV and C IV doublets have the same three velocity components at cz = 1369, 1417, and 1530 km/s found in Ca II H & K, Na I D, Mg I, Mg II, and Fe II, implying that the low and high ionization gas are both found in three "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0409448","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0409448/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":"astro-ph/0409448","created_at":"2026-07-04T16:44:43.128428+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0409448v1","created_at":"2026-07-04T16:44:43.128428+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0409448","created_at":"2026-07-04T16:44:43.128428+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZPDPLQANNHBM","created_at":"2026-07-04T16:44:43.128428+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZPDPLQANNHBMZ4J4","created_at":"2026-07-04T16:44:43.128428+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZPDPLQAN","created_at":"2026-07-04T16:44:43.128428+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.31546","citing_title":"Tracing Cold Gas in Absorption Across Cosmic Time with the SKA","ref_index":163,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZPDPLQANNHBMZ4J4R62NIUXALV","json":"https://pith.science/pith/ZPDPLQANNHBMZ4J4R62NIUXALV.json","graph_json":"https://pith.science/api/pith-number/ZPDPLQANNHBMZ4J4R62NIUXALV/graph.json","events_json":"https://pith.science/api/pith-number/ZPDPLQANNHBMZ4J4R62NIUXALV/events.json","paper":"https://pith.science/paper/ZPDPLQAN"},"agent_actions":{"view_html":"https://pith.science/pith/ZPDPLQANNHBMZ4J4R62NIUXALV","download_json":"https://pith.science/pith/ZPDPLQANNHBMZ4J4R62NIUXALV.json","view_paper":"https://pith.science/paper/ZPDPLQAN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0409448&json=true","fetch_graph":"https://pith.science/api/pith-number/ZPDPLQANNHBMZ4J4R62NIUXALV/graph.json","fetch_events":"https://pith.science/api/pith-number/ZPDPLQANNHBMZ4J4R62NIUXALV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZPDPLQANNHBMZ4J4R62NIUXALV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZPDPLQANNHBMZ4J4R62NIUXALV/action/storage_attestation","attest_author":"https://pith.science/pith/ZPDPLQANNHBMZ4J4R62NIUXALV/action/author_attestation","sign_citation":"https://pith.science/pith/ZPDPLQANNHBMZ4J4R62NIUXALV/action/citation_signature","submit_replication":"https://pith.science/pith/ZPDPLQANNHBMZ4J4R62NIUXALV/action/replication_record"}},"created_at":"2026-07-04T16:44:43.128428+00:00","updated_at":"2026-07-04T16:44:43.128428+00:00"}