{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:MBH3S2B5ZKDLWK6GGAWYDFZLMW","short_pith_number":"pith:MBH3S2B5","schema_version":"1.0","canonical_sha256":"604fb9683dca86bb2bc6302d81972b65b92af4e32f1474838fcd40c707bf7a68","source":{"kind":"arxiv","id":"1802.03423","version":1},"attestation_state":"computed","paper":{"title":"The WISSH Quasars Project IV. BLR versus kpc-scale winds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bongiorno, A. Comastri, A. Marconi, C. Feruglio, C. Vignali, E. Giallongo, E. Piconcelli, E. Sani, F. Duras, F. Fiore, F. La Franca, F. Mannucci, F. Ricci, F. Tombesi, G. Bruni, G. Cresci, G. Vietri, L. Zappacosta, M. Bischetti, M. Brusa, S. Bisogni, S. Martocchia, V. Mainieri, V. Testa","submitted_at":"2018-02-09T19:36:21Z","abstract_excerpt":"We have undertaken a multi-band observing program aimed at obtaining a complete census of winds in a sample of WISE/SDSS selected hyper-luminous (WISSH) QSOs at z~2-4. We have analyzed the rest-frame optical (LBT/LUCI and VLT/SINFONI) and UV (SDSS) spectra of 18 randomly selected WISSH QSOs to measure the SMBH mass and study the properties of winds both in the NLR and BLR traced by blueshifted/skewed [OIII] and CIV emission lines, respectively. These WISSH QSOs are powered by SMBH with masses $\\ge$10$^9$ Msun accreting at 0.4<$\\lambda_{Edd}$<3.1. We have found the existence of two sub-populati"},"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":"1802.03423","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-02-09T19:36:21Z","cross_cats_sorted":[],"title_canon_sha256":"4f457860c5965e3d692301336b938c54c6c2b69aa8db7e6dd05da2f67d1e7ba2","abstract_canon_sha256":"9cd38fc5b7b47b59f793475ba02d2e384ef2e28221bf2d359c50a9d029e9a410"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:04:49.813246Z","signature_b64":"YZqxrZcyhyemPAcQbP/KUOzbiCGXxs84QYrOGQmLtcLy6lhUWN19k5Zif9RmH05AhooC4B21/ZGyW3fLwl5uAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"604fb9683dca86bb2bc6302d81972b65b92af4e32f1474838fcd40c707bf7a68","last_reissued_at":"2026-05-18T00:04:49.812252Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:04:49.812252Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The WISSH Quasars Project IV. BLR versus kpc-scale winds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bongiorno, A. Comastri, A. Marconi, C. Feruglio, C. Vignali, E. Giallongo, E. Piconcelli, E. Sani, F. Duras, F. Fiore, F. La Franca, F. Mannucci, F. Ricci, F. Tombesi, G. Bruni, G. Cresci, G. Vietri, L. Zappacosta, M. Bischetti, M. Brusa, S. Bisogni, S. Martocchia, V. Mainieri, V. Testa","submitted_at":"2018-02-09T19:36:21Z","abstract_excerpt":"We have undertaken a multi-band observing program aimed at obtaining a complete census of winds in a sample of WISE/SDSS selected hyper-luminous (WISSH) QSOs at z~2-4. We have analyzed the rest-frame optical (LBT/LUCI and VLT/SINFONI) and UV (SDSS) spectra of 18 randomly selected WISSH QSOs to measure the SMBH mass and study the properties of winds both in the NLR and BLR traced by blueshifted/skewed [OIII] and CIV emission lines, respectively. These WISSH QSOs are powered by SMBH with masses $\\ge$10$^9$ Msun accreting at 0.4<$\\lambda_{Edd}$<3.1. We have found the existence of two sub-populati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.03423","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":""},"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":"1802.03423","created_at":"2026-05-18T00:04:49.812364+00:00"},{"alias_kind":"arxiv_version","alias_value":"1802.03423v1","created_at":"2026-05-18T00:04:49.812364+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.03423","created_at":"2026-05-18T00:04:49.812364+00:00"},{"alias_kind":"pith_short_12","alias_value":"MBH3S2B5ZKDL","created_at":"2026-05-18T12:32:37.024351+00:00"},{"alias_kind":"pith_short_16","alias_value":"MBH3S2B5ZKDLWK6G","created_at":"2026-05-18T12:32:37.024351+00:00"},{"alias_kind":"pith_short_8","alias_value":"MBH3S2B5","created_at":"2026-05-18T12:32:37.024351+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/MBH3S2B5ZKDLWK6GGAWYDFZLMW","json":"https://pith.science/pith/MBH3S2B5ZKDLWK6GGAWYDFZLMW.json","graph_json":"https://pith.science/api/pith-number/MBH3S2B5ZKDLWK6GGAWYDFZLMW/graph.json","events_json":"https://pith.science/api/pith-number/MBH3S2B5ZKDLWK6GGAWYDFZLMW/events.json","paper":"https://pith.science/paper/MBH3S2B5"},"agent_actions":{"view_html":"https://pith.science/pith/MBH3S2B5ZKDLWK6GGAWYDFZLMW","download_json":"https://pith.science/pith/MBH3S2B5ZKDLWK6GGAWYDFZLMW.json","view_paper":"https://pith.science/paper/MBH3S2B5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1802.03423&json=true","fetch_graph":"https://pith.science/api/pith-number/MBH3S2B5ZKDLWK6GGAWYDFZLMW/graph.json","fetch_events":"https://pith.science/api/pith-number/MBH3S2B5ZKDLWK6GGAWYDFZLMW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MBH3S2B5ZKDLWK6GGAWYDFZLMW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MBH3S2B5ZKDLWK6GGAWYDFZLMW/action/storage_attestation","attest_author":"https://pith.science/pith/MBH3S2B5ZKDLWK6GGAWYDFZLMW/action/author_attestation","sign_citation":"https://pith.science/pith/MBH3S2B5ZKDLWK6GGAWYDFZLMW/action/citation_signature","submit_replication":"https://pith.science/pith/MBH3S2B5ZKDLWK6GGAWYDFZLMW/action/replication_record"}},"created_at":"2026-05-18T00:04:49.812364+00:00","updated_at":"2026-05-18T00:04:49.812364+00:00"}