{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:ZGGES35OLASGENHB4TZMZF6XN6","short_pith_number":"pith:ZGGES35O","schema_version":"1.0","canonical_sha256":"c98c496fae58246234e1e4f2cc97d76fa356f0ea0750c3c0359a76a81e56944b","source":{"kind":"arxiv","id":"2606.26305","version":1},"attestation_state":"computed","paper":{"title":"Wind Acceleration as a Driver of Detached Blueshifted Absorption in Quasar Disk Winds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anna Ritchie, Daniel Proga, Kara Smith, Liliana Flores, Morrigan Kalet, Paola Rodr\\'iguez Hidalgo, Randall C. Dannen","submitted_at":"2026-06-24T18:50:50Z","abstract_excerpt":"Active galactic nuclei (AGN) unification models often emphasize the viewing angle, $i$, but $i$ alone does not determine quasar properties. This is crucial for quasar outflows: UV absorption in Extremely High Velocity Outflow (EHVO) quasars can reach blueshifted velocities of $\\sim0.2~c$. In disk-wind models, both $i$ and internal wind structure shape the emergent spectrum. We test their interplay using biconical quasar disk-wind models with different acceleration lengths, $R_v$, and generate synthetic spectra over a range of $i$. We use Monte Carlo radiative transfer to account for finite con"},"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":"2606.26305","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2026-06-24T18:50:50Z","cross_cats_sorted":[],"title_canon_sha256":"ffe512de7624449e7fc23846842387c6d0ad9d00bfac6a2cf6d2688496a07efd","abstract_canon_sha256":"19716fc155574855898e2ac9f97ca5d24d84f5159583529c381bfa30f6bfb1c6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-26T00:15:36.126052Z","signature_b64":"rUE5mZiSyyQR0Y1Xy/VAwldLWeo2YO5MHLCNOyJc0qLc91Tio6U5hmnaKZiobDEIz461vDUexSlFJQNDi8NmAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c98c496fae58246234e1e4f2cc97d76fa356f0ea0750c3c0359a76a81e56944b","last_reissued_at":"2026-06-26T00:15:36.125570Z","signature_status":"signed_v1","first_computed_at":"2026-06-26T00:15:36.125570Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Wind Acceleration as a Driver of Detached Blueshifted Absorption in Quasar Disk Winds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anna Ritchie, Daniel Proga, Kara Smith, Liliana Flores, Morrigan Kalet, Paola Rodr\\'iguez Hidalgo, Randall C. Dannen","submitted_at":"2026-06-24T18:50:50Z","abstract_excerpt":"Active galactic nuclei (AGN) unification models often emphasize the viewing angle, $i$, but $i$ alone does not determine quasar properties. This is crucial for quasar outflows: UV absorption in Extremely High Velocity Outflow (EHVO) quasars can reach blueshifted velocities of $\\sim0.2~c$. In disk-wind models, both $i$ and internal wind structure shape the emergent spectrum. We test their interplay using biconical quasar disk-wind models with different acceleration lengths, $R_v$, and generate synthetic spectra over a range of $i$. We use Monte Carlo radiative transfer to account for finite con"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.26305","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/2606.26305/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":"2606.26305","created_at":"2026-06-26T00:15:36.125636+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.26305v1","created_at":"2026-06-26T00:15:36.125636+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.26305","created_at":"2026-06-26T00:15:36.125636+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZGGES35OLASG","created_at":"2026-06-26T00:15:36.125636+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZGGES35OLASGENHB","created_at":"2026-06-26T00:15:36.125636+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZGGES35O","created_at":"2026-06-26T00:15:36.125636+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/ZGGES35OLASGENHB4TZMZF6XN6","json":"https://pith.science/pith/ZGGES35OLASGENHB4TZMZF6XN6.json","graph_json":"https://pith.science/api/pith-number/ZGGES35OLASGENHB4TZMZF6XN6/graph.json","events_json":"https://pith.science/api/pith-number/ZGGES35OLASGENHB4TZMZF6XN6/events.json","paper":"https://pith.science/paper/ZGGES35O"},"agent_actions":{"view_html":"https://pith.science/pith/ZGGES35OLASGENHB4TZMZF6XN6","download_json":"https://pith.science/pith/ZGGES35OLASGENHB4TZMZF6XN6.json","view_paper":"https://pith.science/paper/ZGGES35O","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.26305&json=true","fetch_graph":"https://pith.science/api/pith-number/ZGGES35OLASGENHB4TZMZF6XN6/graph.json","fetch_events":"https://pith.science/api/pith-number/ZGGES35OLASGENHB4TZMZF6XN6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZGGES35OLASGENHB4TZMZF6XN6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZGGES35OLASGENHB4TZMZF6XN6/action/storage_attestation","attest_author":"https://pith.science/pith/ZGGES35OLASGENHB4TZMZF6XN6/action/author_attestation","sign_citation":"https://pith.science/pith/ZGGES35OLASGENHB4TZMZF6XN6/action/citation_signature","submit_replication":"https://pith.science/pith/ZGGES35OLASGENHB4TZMZF6XN6/action/replication_record"}},"created_at":"2026-06-26T00:15:36.125636+00:00","updated_at":"2026-06-26T00:15:36.125636+00:00"}