{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:OPQSE6G5QVFJ3HIOY6YU4UAPDI","short_pith_number":"pith:OPQSE6G5","schema_version":"1.0","canonical_sha256":"73e12278dd854a9d9d0ec7b14e500f1a28b3d7ddc7dc35ba4a7d81bafdb41261","source":{"kind":"arxiv","id":"2412.06929","version":3},"attestation_state":"computed","paper":{"title":"Physical characterization of the FeLoBAL outflow in SDSS J0932+0840: Analysis of VLT/UVES observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Doyee Byun, Gwen Walker, Kirk T. Korista, Manuel Bautista, Maryam Dehghanian, Mayank Sharma, Nahum Arav, Sasha Mintz","submitted_at":"2024-12-09T19:15:22Z","abstract_excerpt":"Context: The study of quasar outflows is essential in understanding the connection between active galactic nuclei (AGN) and their host galaxies. We analyze the VLT/UVES spectrum of quasar SDSS J0932+0840 and identify several narrow and broad outflow components in absorption, with multiple ionization species including Fe II, which puts it among a rare class of outflows known as FeLoBALs. Aims: We study one of the outflow components to determine its physical characteristics by determining the total hydrogen column density, ionization parameter and the hydrogen number density. Through these param"},"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":"2412.06929","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-12-09T19:15:22Z","cross_cats_sorted":[],"title_canon_sha256":"81999f8017af87bb5b31a01473815c1080f8c11133e0d3351d43040b2d17e232","abstract_canon_sha256":"59d88b9777251b24e9968a206c86b5107ef8c18e19d52d02772603b81c70c1cf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:06:31.844157Z","signature_b64":"1IYm9NWEWXzx5/jand22DP6sfjZkcOvlww9Iah25+OWRrWD8QAYJMB1aa99LzGEtkA9bi9uph/ZvH7bv9M8gDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"73e12278dd854a9d9d0ec7b14e500f1a28b3d7ddc7dc35ba4a7d81bafdb41261","last_reissued_at":"2026-07-05T10:06:31.843686Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:06:31.843686Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Physical characterization of the FeLoBAL outflow in SDSS J0932+0840: Analysis of VLT/UVES observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Doyee Byun, Gwen Walker, Kirk T. Korista, Manuel Bautista, Maryam Dehghanian, Mayank Sharma, Nahum Arav, Sasha Mintz","submitted_at":"2024-12-09T19:15:22Z","abstract_excerpt":"Context: The study of quasar outflows is essential in understanding the connection between active galactic nuclei (AGN) and their host galaxies. We analyze the VLT/UVES spectrum of quasar SDSS J0932+0840 and identify several narrow and broad outflow components in absorption, with multiple ionization species including Fe II, which puts it among a rare class of outflows known as FeLoBALs. Aims: We study one of the outflow components to determine its physical characteristics by determining the total hydrogen column density, ionization parameter and the hydrogen number density. Through these param"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.06929","kind":"arxiv","version":3},"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/2412.06929/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":"2412.06929","created_at":"2026-07-05T10:06:31.843740+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.06929v3","created_at":"2026-07-05T10:06:31.843740+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.06929","created_at":"2026-07-05T10:06:31.843740+00:00"},{"alias_kind":"pith_short_12","alias_value":"OPQSE6G5QVFJ","created_at":"2026-07-05T10:06:31.843740+00:00"},{"alias_kind":"pith_short_16","alias_value":"OPQSE6G5QVFJ3HIO","created_at":"2026-07-05T10:06:31.843740+00:00"},{"alias_kind":"pith_short_8","alias_value":"OPQSE6G5","created_at":"2026-07-05T10:06:31.843740+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/OPQSE6G5QVFJ3HIOY6YU4UAPDI","json":"https://pith.science/pith/OPQSE6G5QVFJ3HIOY6YU4UAPDI.json","graph_json":"https://pith.science/api/pith-number/OPQSE6G5QVFJ3HIOY6YU4UAPDI/graph.json","events_json":"https://pith.science/api/pith-number/OPQSE6G5QVFJ3HIOY6YU4UAPDI/events.json","paper":"https://pith.science/paper/OPQSE6G5"},"agent_actions":{"view_html":"https://pith.science/pith/OPQSE6G5QVFJ3HIOY6YU4UAPDI","download_json":"https://pith.science/pith/OPQSE6G5QVFJ3HIOY6YU4UAPDI.json","view_paper":"https://pith.science/paper/OPQSE6G5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.06929&json=true","fetch_graph":"https://pith.science/api/pith-number/OPQSE6G5QVFJ3HIOY6YU4UAPDI/graph.json","fetch_events":"https://pith.science/api/pith-number/OPQSE6G5QVFJ3HIOY6YU4UAPDI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OPQSE6G5QVFJ3HIOY6YU4UAPDI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OPQSE6G5QVFJ3HIOY6YU4UAPDI/action/storage_attestation","attest_author":"https://pith.science/pith/OPQSE6G5QVFJ3HIOY6YU4UAPDI/action/author_attestation","sign_citation":"https://pith.science/pith/OPQSE6G5QVFJ3HIOY6YU4UAPDI/action/citation_signature","submit_replication":"https://pith.science/pith/OPQSE6G5QVFJ3HIOY6YU4UAPDI/action/replication_record"}},"created_at":"2026-07-05T10:06:31.843740+00:00","updated_at":"2026-07-05T10:06:31.843740+00:00"}