{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:X3VBAVQQLYLQQTESBSGZG4T3X5","short_pith_number":"pith:X3VBAVQQ","schema_version":"1.0","canonical_sha256":"beea1056105e17084c920c8d93727bbf6f174f498c02e572b32cfb55cea5ac41","source":{"kind":"arxiv","id":"2101.04688","version":2},"attestation_state":"computed","paper":{"title":"Powerful winds in high-redshift obscured and red quasars","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andrey Vayner, David S. N. Rupke, Dominika Wylezalek, Fred Hamann, Greg Walth, Maren Cosens, Nadia L. Zakamska, Rachael Alexandroff, Rogemar A. Riffel, Serena Perrotta, Shelley Wright, Sylvain Veilleux, Thaisa Storchi Bergmann","submitted_at":"2021-01-12T19:00:01Z","abstract_excerpt":"Quasar-driven outflows must have made their most significant impact on galaxy formation during the epoch when massive galaxies were forming most rapidly. To study the impact of quasar feedback we conducted rest-frame optical integral field spectrograph (IFS) observations of three extremely red quasars (ERQs) and one type-2 quasar at $z=2-3$, obtained with the NIFS and OSIRIS instruments at the Gemini North and W. M. Keck Observatory with the assistance of laser-guided adaptive optics. We use the kinematics and morphologies of the [OIII] 5007\\AA and H$\\alpha$ 6563\\AA emission lines redshifted i"},"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":"2101.04688","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2021-01-12T19:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"fd6703b346d2fcf2353586c6899167190e0c8e7718e7a029b7192fb415ba429d","abstract_canon_sha256":"bdd66c5645c2a099417a13072f5b4c721e6907b8536a63119d29231e9435361d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:47:03.912700Z","signature_b64":"C55YaB7xneiI/OXPRkYQnH8O7fpR6a1mc3HwhbH2FZpw1nqbfz2ZSwl2WYJ71BCVCFhhXbs4OSVHO5E7FKn7CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"beea1056105e17084c920c8d93727bbf6f174f498c02e572b32cfb55cea5ac41","last_reissued_at":"2026-07-05T02:47:03.912139Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:47:03.912139Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Powerful winds in high-redshift obscured and red quasars","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andrey Vayner, David S. N. Rupke, Dominika Wylezalek, Fred Hamann, Greg Walth, Maren Cosens, Nadia L. Zakamska, Rachael Alexandroff, Rogemar A. Riffel, Serena Perrotta, Shelley Wright, Sylvain Veilleux, Thaisa Storchi Bergmann","submitted_at":"2021-01-12T19:00:01Z","abstract_excerpt":"Quasar-driven outflows must have made their most significant impact on galaxy formation during the epoch when massive galaxies were forming most rapidly. To study the impact of quasar feedback we conducted rest-frame optical integral field spectrograph (IFS) observations of three extremely red quasars (ERQs) and one type-2 quasar at $z=2-3$, obtained with the NIFS and OSIRIS instruments at the Gemini North and W. M. Keck Observatory with the assistance of laser-guided adaptive optics. We use the kinematics and morphologies of the [OIII] 5007\\AA and H$\\alpha$ 6563\\AA emission lines redshifted i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2101.04688","kind":"arxiv","version":2},"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/2101.04688/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":"2101.04688","created_at":"2026-07-05T02:47:03.912195+00:00"},{"alias_kind":"arxiv_version","alias_value":"2101.04688v2","created_at":"2026-07-05T02:47:03.912195+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2101.04688","created_at":"2026-07-05T02:47:03.912195+00:00"},{"alias_kind":"pith_short_12","alias_value":"X3VBAVQQLYLQ","created_at":"2026-07-05T02:47:03.912195+00:00"},{"alias_kind":"pith_short_16","alias_value":"X3VBAVQQLYLQQTES","created_at":"2026-07-05T02:47:03.912195+00:00"},{"alias_kind":"pith_short_8","alias_value":"X3VBAVQQ","created_at":"2026-07-05T02:47:03.912195+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/X3VBAVQQLYLQQTESBSGZG4T3X5","json":"https://pith.science/pith/X3VBAVQQLYLQQTESBSGZG4T3X5.json","graph_json":"https://pith.science/api/pith-number/X3VBAVQQLYLQQTESBSGZG4T3X5/graph.json","events_json":"https://pith.science/api/pith-number/X3VBAVQQLYLQQTESBSGZG4T3X5/events.json","paper":"https://pith.science/paper/X3VBAVQQ"},"agent_actions":{"view_html":"https://pith.science/pith/X3VBAVQQLYLQQTESBSGZG4T3X5","download_json":"https://pith.science/pith/X3VBAVQQLYLQQTESBSGZG4T3X5.json","view_paper":"https://pith.science/paper/X3VBAVQQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2101.04688&json=true","fetch_graph":"https://pith.science/api/pith-number/X3VBAVQQLYLQQTESBSGZG4T3X5/graph.json","fetch_events":"https://pith.science/api/pith-number/X3VBAVQQLYLQQTESBSGZG4T3X5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X3VBAVQQLYLQQTESBSGZG4T3X5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X3VBAVQQLYLQQTESBSGZG4T3X5/action/storage_attestation","attest_author":"https://pith.science/pith/X3VBAVQQLYLQQTESBSGZG4T3X5/action/author_attestation","sign_citation":"https://pith.science/pith/X3VBAVQQLYLQQTESBSGZG4T3X5/action/citation_signature","submit_replication":"https://pith.science/pith/X3VBAVQQLYLQQTESBSGZG4T3X5/action/replication_record"}},"created_at":"2026-07-05T02:47:03.912195+00:00","updated_at":"2026-07-05T02:47:03.912195+00:00"}