{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:RMMCD7TBVMWZPMTV3HEGTHGMYL","short_pith_number":"pith:RMMCD7TB","schema_version":"1.0","canonical_sha256":"8b1821fe61ab2d97b275d9c8699cccc2fe566609e136aa2c8558311ed2ff0d2d","source":{"kind":"arxiv","id":"astro-ph/0604091","version":1},"attestation_state":"computed","paper":{"title":"A Survey of O VI, C III, and H I in Highly Ionized High-Velocity Clouds","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Andrew J. Fox, Bart P. Wakker, Blair D. Savage","submitted_at":"2006-04-05T15:46:57Z","abstract_excerpt":"(ABRIDGED) We present a Far-Ultraviolet Spectroscopic Explorer survey of highly ionized high-velocity clouds (HVCs) in 66 extragalactic sight lines. We find a total of 63 high-velocity O VI absorbers, 16 with 21 cm-emitting H I counterparts and 47 ``highly ionized'' absorbers without 21 cm emission. 11 of these high-velocity O VI absorbers are positive-velocity wings (broad O VI features extending asymmetrically to velocities of up to 300 km/s). The highly ionized HVC population is characterized by <b(O VI)>=38+/-10 km/s and <log N_a(O VI)>=13.83+/-0.36. We find that 81% (30/37) of high-veloci"},"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/0604091","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-04-05T15:46:57Z","cross_cats_sorted":[],"title_canon_sha256":"5bd4b6d2715af2381fefea40ff310bef944d63d120aff9e460cf4172e0a43a9e","abstract_canon_sha256":"6dded871f0fd253d5ebca3129a164c67e4bc8e0471eee87cab0a4e0daeec8712"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:58:33.720900Z","signature_b64":"1FojiTlv6cGBeMGfHL6m5mR3+jxVc/ldLoz5QA97kMewInsjtbtEgtuX3GQEkcICHfrd5Pla3c+rnvRycaiEAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8b1821fe61ab2d97b275d9c8699cccc2fe566609e136aa2c8558311ed2ff0d2d","last_reissued_at":"2026-07-04T16:58:33.720457Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:58:33.720457Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Survey of O VI, C III, and H I in Highly Ionized High-Velocity Clouds","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Andrew J. Fox, Bart P. Wakker, Blair D. Savage","submitted_at":"2006-04-05T15:46:57Z","abstract_excerpt":"(ABRIDGED) We present a Far-Ultraviolet Spectroscopic Explorer survey of highly ionized high-velocity clouds (HVCs) in 66 extragalactic sight lines. We find a total of 63 high-velocity O VI absorbers, 16 with 21 cm-emitting H I counterparts and 47 ``highly ionized'' absorbers without 21 cm emission. 11 of these high-velocity O VI absorbers are positive-velocity wings (broad O VI features extending asymmetrically to velocities of up to 300 km/s). The highly ionized HVC population is characterized by <b(O VI)>=38+/-10 km/s and <log N_a(O VI)>=13.83+/-0.36. We find that 81% (30/37) of high-veloci"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0604091","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/0604091/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/0604091","created_at":"2026-07-04T16:58:33.720518+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0604091v1","created_at":"2026-07-04T16:58:33.720518+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0604091","created_at":"2026-07-04T16:58:33.720518+00:00"},{"alias_kind":"pith_short_12","alias_value":"RMMCD7TBVMWZ","created_at":"2026-07-04T16:58:33.720518+00:00"},{"alias_kind":"pith_short_16","alias_value":"RMMCD7TBVMWZPMTV","created_at":"2026-07-04T16:58:33.720518+00:00"},{"alias_kind":"pith_short_8","alias_value":"RMMCD7TB","created_at":"2026-07-04T16:58:33.720518+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.11506","citing_title":"Revealing Cosmic Ecosystems with the Hubble Space Telescope in 2030s and Beyond","ref_index":14,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RMMCD7TBVMWZPMTV3HEGTHGMYL","json":"https://pith.science/pith/RMMCD7TBVMWZPMTV3HEGTHGMYL.json","graph_json":"https://pith.science/api/pith-number/RMMCD7TBVMWZPMTV3HEGTHGMYL/graph.json","events_json":"https://pith.science/api/pith-number/RMMCD7TBVMWZPMTV3HEGTHGMYL/events.json","paper":"https://pith.science/paper/RMMCD7TB"},"agent_actions":{"view_html":"https://pith.science/pith/RMMCD7TBVMWZPMTV3HEGTHGMYL","download_json":"https://pith.science/pith/RMMCD7TBVMWZPMTV3HEGTHGMYL.json","view_paper":"https://pith.science/paper/RMMCD7TB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0604091&json=true","fetch_graph":"https://pith.science/api/pith-number/RMMCD7TBVMWZPMTV3HEGTHGMYL/graph.json","fetch_events":"https://pith.science/api/pith-number/RMMCD7TBVMWZPMTV3HEGTHGMYL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RMMCD7TBVMWZPMTV3HEGTHGMYL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RMMCD7TBVMWZPMTV3HEGTHGMYL/action/storage_attestation","attest_author":"https://pith.science/pith/RMMCD7TBVMWZPMTV3HEGTHGMYL/action/author_attestation","sign_citation":"https://pith.science/pith/RMMCD7TBVMWZPMTV3HEGTHGMYL/action/citation_signature","submit_replication":"https://pith.science/pith/RMMCD7TBVMWZPMTV3HEGTHGMYL/action/replication_record"}},"created_at":"2026-07-04T16:58:33.720518+00:00","updated_at":"2026-07-04T16:58:33.720518+00:00"}