{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:I6Q3QJT3SQ4POVLSNGBF323YHS","short_pith_number":"pith:I6Q3QJT3","schema_version":"1.0","canonical_sha256":"47a1b8267b9438f7557269825deb783c9fec2f9623653b3125807677b2ffad3c","source":{"kind":"arxiv","id":"1002.4681","version":1},"attestation_state":"computed","paper":{"title":"The Redshifted Excess in Quasar C IV Broad Emission Lines","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Brian Punsly","submitted_at":"2010-02-25T02:32:36Z","abstract_excerpt":"In this Letter, the Evans and Koratkar Atlas of Hubble Space Telescope Faint Object Spectrograph Spectra of Active Galactic Nuclei and Quasars is used to study the redward asymmetry in CIV broad emission lines (BELs). It is concluded that there is a highly significant correlation between the spectral index from 10 GHz to 1350 $\\AA$ and the amount of excess luminosity in the red wing of the CIV BEL ($>99.9999%$ significance level for the full sample and the radio loud subsample independently, but no correlation is found for the radio quiet subsample). This is interpreted as a correlation betwee"},"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":"1002.4681","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-02-25T02:32:36Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"85a8360e5520d3075ecbd6e80b8c3404a2c9630a2c36f8162257dccd71046b4c","abstract_canon_sha256":"4cd6c272f58b72b8444a61b86770629f071e99598212e05401e8a0697e15fe72"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:08:57.055062Z","signature_b64":"hWJSPxWDwbyC/vbRKaSgAQ2t6ofBe2O1rX+Y/E1cEEh2+GNt8GKBoupfG8L+upcaiZZodPtEVfPORFTl6lP0Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"47a1b8267b9438f7557269825deb783c9fec2f9623653b3125807677b2ffad3c","last_reissued_at":"2026-05-18T02:08:57.052569Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:08:57.052569Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Redshifted Excess in Quasar C IV Broad Emission Lines","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Brian Punsly","submitted_at":"2010-02-25T02:32:36Z","abstract_excerpt":"In this Letter, the Evans and Koratkar Atlas of Hubble Space Telescope Faint Object Spectrograph Spectra of Active Galactic Nuclei and Quasars is used to study the redward asymmetry in CIV broad emission lines (BELs). It is concluded that there is a highly significant correlation between the spectral index from 10 GHz to 1350 $\\AA$ and the amount of excess luminosity in the red wing of the CIV BEL ($>99.9999%$ significance level for the full sample and the radio loud subsample independently, but no correlation is found for the radio quiet subsample). This is interpreted as a correlation betwee"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1002.4681","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":"1002.4681","created_at":"2026-05-18T02:08:57.052691+00:00"},{"alias_kind":"arxiv_version","alias_value":"1002.4681v1","created_at":"2026-05-18T02:08:57.052691+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1002.4681","created_at":"2026-05-18T02:08:57.052691+00:00"},{"alias_kind":"pith_short_12","alias_value":"I6Q3QJT3SQ4P","created_at":"2026-05-18T12:26:07.630475+00:00"},{"alias_kind":"pith_short_16","alias_value":"I6Q3QJT3SQ4POVLS","created_at":"2026-05-18T12:26:07.630475+00:00"},{"alias_kind":"pith_short_8","alias_value":"I6Q3QJT3","created_at":"2026-05-18T12:26:07.630475+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/I6Q3QJT3SQ4POVLSNGBF323YHS","json":"https://pith.science/pith/I6Q3QJT3SQ4POVLSNGBF323YHS.json","graph_json":"https://pith.science/api/pith-number/I6Q3QJT3SQ4POVLSNGBF323YHS/graph.json","events_json":"https://pith.science/api/pith-number/I6Q3QJT3SQ4POVLSNGBF323YHS/events.json","paper":"https://pith.science/paper/I6Q3QJT3"},"agent_actions":{"view_html":"https://pith.science/pith/I6Q3QJT3SQ4POVLSNGBF323YHS","download_json":"https://pith.science/pith/I6Q3QJT3SQ4POVLSNGBF323YHS.json","view_paper":"https://pith.science/paper/I6Q3QJT3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1002.4681&json=true","fetch_graph":"https://pith.science/api/pith-number/I6Q3QJT3SQ4POVLSNGBF323YHS/graph.json","fetch_events":"https://pith.science/api/pith-number/I6Q3QJT3SQ4POVLSNGBF323YHS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I6Q3QJT3SQ4POVLSNGBF323YHS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I6Q3QJT3SQ4POVLSNGBF323YHS/action/storage_attestation","attest_author":"https://pith.science/pith/I6Q3QJT3SQ4POVLSNGBF323YHS/action/author_attestation","sign_citation":"https://pith.science/pith/I6Q3QJT3SQ4POVLSNGBF323YHS/action/citation_signature","submit_replication":"https://pith.science/pith/I6Q3QJT3SQ4POVLSNGBF323YHS/action/replication_record"}},"created_at":"2026-05-18T02:08:57.052691+00:00","updated_at":"2026-05-18T02:08:57.052691+00:00"}