{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:DJE3EI5CBBXBWCKA4ZFH6FW5KO","short_pith_number":"pith:DJE3EI5C","schema_version":"1.0","canonical_sha256":"1a49b223a2086e1b0940e64a7f16dd53b545b266ac06f8c1c317dfacadd9fc7a","source":{"kind":"arxiv","id":"1201.5155","version":1},"attestation_state":"computed","paper":{"title":"Updating quasar bolometric luminosity corrections","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Jessie C. Runnoe, Michael S. Brotherton, Zhaohui Shang","submitted_at":"2012-01-24T23:22:57Z","abstract_excerpt":"Bolometric corrections are used in quasar studies to quantify total energy output based on a measurement of a monochromatic luminosity. First, we enumerate and discuss the practical difficulties of determining such corrections, then we present bolometric luminosities between 1 \\mu m and 8 keV rest frame and corrections derived from the detailed spectral energy distributions of 63 bright quasars of low to moderate redshift (z = 0.03-1.4). Exploring several mathematical fittings, we provide practical bolometric corrections of the forms L_iso=\\zeta \\lambda L_{\\lambda} and log(L_iso)=A+B log(\\lamb"},"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":"1201.5155","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-01-24T23:22:57Z","cross_cats_sorted":[],"title_canon_sha256":"e083df2e5faf6756fc30347621cdd448ebdb76ad52afa816b084e7a44be15902","abstract_canon_sha256":"3e8514f636b6d53f5dbcb601268f70249f484560cce60c6f02652bcd3e55590d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:42.329228Z","signature_b64":"FtZTM4xcuorpMzgKxpXDyz0dt2tcAuPxCc7x1mmtE/n72nXVltE6Hx0u+Y6n9BPa4KbeUHC0bIoSYR5KwxK1AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1a49b223a2086e1b0940e64a7f16dd53b545b266ac06f8c1c317dfacadd9fc7a","last_reissued_at":"2026-05-18T01:58:42.328598Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:42.328598Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Updating quasar bolometric luminosity corrections","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Jessie C. Runnoe, Michael S. Brotherton, Zhaohui Shang","submitted_at":"2012-01-24T23:22:57Z","abstract_excerpt":"Bolometric corrections are used in quasar studies to quantify total energy output based on a measurement of a monochromatic luminosity. First, we enumerate and discuss the practical difficulties of determining such corrections, then we present bolometric luminosities between 1 \\mu m and 8 keV rest frame and corrections derived from the detailed spectral energy distributions of 63 bright quasars of low to moderate redshift (z = 0.03-1.4). Exploring several mathematical fittings, we provide practical bolometric corrections of the forms L_iso=\\zeta \\lambda L_{\\lambda} and log(L_iso)=A+B log(\\lamb"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.5155","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":"1201.5155","created_at":"2026-05-18T01:58:42.328686+00:00"},{"alias_kind":"arxiv_version","alias_value":"1201.5155v1","created_at":"2026-05-18T01:58:42.328686+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.5155","created_at":"2026-05-18T01:58:42.328686+00:00"},{"alias_kind":"pith_short_12","alias_value":"DJE3EI5CBBXB","created_at":"2026-05-18T12:27:04.183437+00:00"},{"alias_kind":"pith_short_16","alias_value":"DJE3EI5CBBXBWCKA","created_at":"2026-05-18T12:27:04.183437+00:00"},{"alias_kind":"pith_short_8","alias_value":"DJE3EI5C","created_at":"2026-05-18T12:27:04.183437+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/DJE3EI5CBBXBWCKA4ZFH6FW5KO","json":"https://pith.science/pith/DJE3EI5CBBXBWCKA4ZFH6FW5KO.json","graph_json":"https://pith.science/api/pith-number/DJE3EI5CBBXBWCKA4ZFH6FW5KO/graph.json","events_json":"https://pith.science/api/pith-number/DJE3EI5CBBXBWCKA4ZFH6FW5KO/events.json","paper":"https://pith.science/paper/DJE3EI5C"},"agent_actions":{"view_html":"https://pith.science/pith/DJE3EI5CBBXBWCKA4ZFH6FW5KO","download_json":"https://pith.science/pith/DJE3EI5CBBXBWCKA4ZFH6FW5KO.json","view_paper":"https://pith.science/paper/DJE3EI5C","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1201.5155&json=true","fetch_graph":"https://pith.science/api/pith-number/DJE3EI5CBBXBWCKA4ZFH6FW5KO/graph.json","fetch_events":"https://pith.science/api/pith-number/DJE3EI5CBBXBWCKA4ZFH6FW5KO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DJE3EI5CBBXBWCKA4ZFH6FW5KO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DJE3EI5CBBXBWCKA4ZFH6FW5KO/action/storage_attestation","attest_author":"https://pith.science/pith/DJE3EI5CBBXBWCKA4ZFH6FW5KO/action/author_attestation","sign_citation":"https://pith.science/pith/DJE3EI5CBBXBWCKA4ZFH6FW5KO/action/citation_signature","submit_replication":"https://pith.science/pith/DJE3EI5CBBXBWCKA4ZFH6FW5KO/action/replication_record"}},"created_at":"2026-05-18T01:58:42.328686+00:00","updated_at":"2026-05-18T01:58:42.328686+00:00"}