{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:DEGAUFWOA3QANRM3UXNGBYJVUL","short_pith_number":"pith:DEGAUFWO","schema_version":"1.0","canonical_sha256":"190c0a16ce06e006c59ba5da60e135a2c311816401ca168cd163e2c479ed81ef","source":{"kind":"arxiv","id":"0910.5256","version":1},"attestation_state":"computed","paper":{"title":"The power output of local obscured and unobscured AGN: crossing the absorption barrier with Swift/BAT and IRAS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"A. C. Fabian, L. M. Winter, P. Gandhi, R. F. Mushotzky, R. V. Vasudevan","submitted_at":"2009-10-27T22:03:25Z","abstract_excerpt":"The Swift/BAT 9-month catalogue of active galactic nuclei (AGN) provides an unbiased census of local supermassive black hole accretion, and probes to all but the highest levels of absorption in AGN. We explore a method for characterising the bolometric output of both obscured and unobscured AGN by combining the hard X-ray data from Swift/BAT (14-195keV) with the reprocessed IR emission as seen with the IRAS all-sky surveys. This approach bypasses the complex modifications to the SED introduced by absorption in the optical, UV and 0.1-10 keV regimes and provides a long-term, average picture of "},"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":"0910.5256","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2009-10-27T22:03:25Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"558fe91e0373567f66b5c004782d6efd525ef555f3dba75d4cb91513e1023a58","abstract_canon_sha256":"7b1e406d9a6dd4d70b69bc4a771854282d95077035d88811bb107973c93a6950"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:11:10.672443Z","signature_b64":"khCjcmiLdGr/+bz2ggyeYx1eB9NNXUV+nenUCOQzonwLFO6zAf9fJ28qTno4QPc4gxpu1rmYo79GGKo/HHdKAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"190c0a16ce06e006c59ba5da60e135a2c311816401ca168cd163e2c479ed81ef","last_reissued_at":"2026-05-18T02:11:10.671573Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:11:10.671573Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The power output of local obscured and unobscured AGN: crossing the absorption barrier with Swift/BAT and IRAS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"A. C. Fabian, L. M. Winter, P. Gandhi, R. F. Mushotzky, R. V. Vasudevan","submitted_at":"2009-10-27T22:03:25Z","abstract_excerpt":"The Swift/BAT 9-month catalogue of active galactic nuclei (AGN) provides an unbiased census of local supermassive black hole accretion, and probes to all but the highest levels of absorption in AGN. We explore a method for characterising the bolometric output of both obscured and unobscured AGN by combining the hard X-ray data from Swift/BAT (14-195keV) with the reprocessed IR emission as seen with the IRAS all-sky surveys. This approach bypasses the complex modifications to the SED introduced by absorption in the optical, UV and 0.1-10 keV regimes and provides a long-term, average picture of "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0910.5256","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":"0910.5256","created_at":"2026-05-18T02:11:10.671737+00:00"},{"alias_kind":"arxiv_version","alias_value":"0910.5256v1","created_at":"2026-05-18T02:11:10.671737+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0910.5256","created_at":"2026-05-18T02:11:10.671737+00:00"},{"alias_kind":"pith_short_12","alias_value":"DEGAUFWOA3QA","created_at":"2026-05-18T12:25:59.703012+00:00"},{"alias_kind":"pith_short_16","alias_value":"DEGAUFWOA3QANRM3","created_at":"2026-05-18T12:25:59.703012+00:00"},{"alias_kind":"pith_short_8","alias_value":"DEGAUFWO","created_at":"2026-05-18T12:25:59.703012+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/DEGAUFWOA3QANRM3UXNGBYJVUL","json":"https://pith.science/pith/DEGAUFWOA3QANRM3UXNGBYJVUL.json","graph_json":"https://pith.science/api/pith-number/DEGAUFWOA3QANRM3UXNGBYJVUL/graph.json","events_json":"https://pith.science/api/pith-number/DEGAUFWOA3QANRM3UXNGBYJVUL/events.json","paper":"https://pith.science/paper/DEGAUFWO"},"agent_actions":{"view_html":"https://pith.science/pith/DEGAUFWOA3QANRM3UXNGBYJVUL","download_json":"https://pith.science/pith/DEGAUFWOA3QANRM3UXNGBYJVUL.json","view_paper":"https://pith.science/paper/DEGAUFWO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0910.5256&json=true","fetch_graph":"https://pith.science/api/pith-number/DEGAUFWOA3QANRM3UXNGBYJVUL/graph.json","fetch_events":"https://pith.science/api/pith-number/DEGAUFWOA3QANRM3UXNGBYJVUL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DEGAUFWOA3QANRM3UXNGBYJVUL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DEGAUFWOA3QANRM3UXNGBYJVUL/action/storage_attestation","attest_author":"https://pith.science/pith/DEGAUFWOA3QANRM3UXNGBYJVUL/action/author_attestation","sign_citation":"https://pith.science/pith/DEGAUFWOA3QANRM3UXNGBYJVUL/action/citation_signature","submit_replication":"https://pith.science/pith/DEGAUFWOA3QANRM3UXNGBYJVUL/action/replication_record"}},"created_at":"2026-05-18T02:11:10.671737+00:00","updated_at":"2026-05-18T02:11:10.671737+00:00"}