{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:VXDBNP7ZCX32Z3AHYLSBCXYMVG","short_pith_number":"pith:VXDBNP7Z","schema_version":"1.0","canonical_sha256":"adc616bff915f7acec07c2e4115f0ca98ab50ce5b5cb69cca43ab137d7ff6ca3","source":{"kind":"arxiv","id":"1108.0927","version":3},"attestation_state":"computed","paper":{"title":"The relation between broad lines and gamma--ray luminosities in Fermi blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"G. Ghisellini, L. Maraschi, M. Colpi, T. Sbarrato","submitted_at":"2011-08-03T20:00:02Z","abstract_excerpt":"We study the relation between the mass accretion rate, the jet power, and the black hole mass of blazars. To this aim, we make use of the Sloan Digital Sky Survey (SDSS) and the 11 months catalog of blazars detected at energies larger than 100 MeV by the Large Area Telescope (LAT) onboard the Fermi satellite. This allows to construct a relatively large sample of blazars with information about the luminosity (or upper limits) of their emission lines used as a proxy for the strength of the disc luminosity and on the luminosity of the high energy emission, used as a proxy for the jet power. We fi"},"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":"1108.0927","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-08-03T20:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"9168a73f87e7197ae988913cfccd60d7f02d61f887b39486fc291dc1f823828f","abstract_canon_sha256":"029c8e12a60f1389aba0e29ac0bf2673a5ef8cb7eb3dfd8a90c010ff20d51c63"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:55:24.849081Z","signature_b64":"UjSdj5Zb2wy1j/9PxWlWuN4sLjJ/FU9xaIHXdyR++/JWBn/XcNzGEbxh1K5VDa4jug1alfnlx7xX+p28v8taBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"adc616bff915f7acec07c2e4115f0ca98ab50ce5b5cb69cca43ab137d7ff6ca3","last_reissued_at":"2026-05-18T03:55:24.848327Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:55:24.848327Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The relation between broad lines and gamma--ray luminosities in Fermi blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"G. Ghisellini, L. Maraschi, M. Colpi, T. Sbarrato","submitted_at":"2011-08-03T20:00:02Z","abstract_excerpt":"We study the relation between the mass accretion rate, the jet power, and the black hole mass of blazars. To this aim, we make use of the Sloan Digital Sky Survey (SDSS) and the 11 months catalog of blazars detected at energies larger than 100 MeV by the Large Area Telescope (LAT) onboard the Fermi satellite. This allows to construct a relatively large sample of blazars with information about the luminosity (or upper limits) of their emission lines used as a proxy for the strength of the disc luminosity and on the luminosity of the high energy emission, used as a proxy for the jet power. We fi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.0927","kind":"arxiv","version":3},"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":"1108.0927","created_at":"2026-05-18T03:55:24.848431+00:00"},{"alias_kind":"arxiv_version","alias_value":"1108.0927v3","created_at":"2026-05-18T03:55:24.848431+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.0927","created_at":"2026-05-18T03:55:24.848431+00:00"},{"alias_kind":"pith_short_12","alias_value":"VXDBNP7ZCX32","created_at":"2026-05-18T12:26:44.992195+00:00"},{"alias_kind":"pith_short_16","alias_value":"VXDBNP7ZCX32Z3AH","created_at":"2026-05-18T12:26:44.992195+00:00"},{"alias_kind":"pith_short_8","alias_value":"VXDBNP7Z","created_at":"2026-05-18T12:26:44.992195+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/VXDBNP7ZCX32Z3AHYLSBCXYMVG","json":"https://pith.science/pith/VXDBNP7ZCX32Z3AHYLSBCXYMVG.json","graph_json":"https://pith.science/api/pith-number/VXDBNP7ZCX32Z3AHYLSBCXYMVG/graph.json","events_json":"https://pith.science/api/pith-number/VXDBNP7ZCX32Z3AHYLSBCXYMVG/events.json","paper":"https://pith.science/paper/VXDBNP7Z"},"agent_actions":{"view_html":"https://pith.science/pith/VXDBNP7ZCX32Z3AHYLSBCXYMVG","download_json":"https://pith.science/pith/VXDBNP7ZCX32Z3AHYLSBCXYMVG.json","view_paper":"https://pith.science/paper/VXDBNP7Z","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1108.0927&json=true","fetch_graph":"https://pith.science/api/pith-number/VXDBNP7ZCX32Z3AHYLSBCXYMVG/graph.json","fetch_events":"https://pith.science/api/pith-number/VXDBNP7ZCX32Z3AHYLSBCXYMVG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VXDBNP7ZCX32Z3AHYLSBCXYMVG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VXDBNP7ZCX32Z3AHYLSBCXYMVG/action/storage_attestation","attest_author":"https://pith.science/pith/VXDBNP7ZCX32Z3AHYLSBCXYMVG/action/author_attestation","sign_citation":"https://pith.science/pith/VXDBNP7ZCX32Z3AHYLSBCXYMVG/action/citation_signature","submit_replication":"https://pith.science/pith/VXDBNP7ZCX32Z3AHYLSBCXYMVG/action/replication_record"}},"created_at":"2026-05-18T03:55:24.848431+00:00","updated_at":"2026-05-18T03:55:24.848431+00:00"}