{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:UJ7P4UPORBCIWAYLWZBTYEJSUH","short_pith_number":"pith:UJ7P4UPO","schema_version":"1.0","canonical_sha256":"a27efe51ee88448b030bb6433c1132a1c1a1bf684b26a5e4afd5fe63323deb99","source":{"kind":"arxiv","id":"1404.3556","version":2},"attestation_state":"computed","paper":{"title":"Intrinsic $\\gamma$-ray luminosity, black hole mass, jet and accretion in Fermi blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Dingrong Xiong, Xiong Zhang","submitted_at":"2014-04-14T12:41:37Z","abstract_excerpt":"We have analyzed a large sample of clean blazars detected by Fermi Large Area Telescope (LAT). Using literature and calculation, we obtained intrinsic $\\gamma$-ray luminosity excluding beaming effect, black hole mass, broad-line luminosity (used as a proxy for disk luminosity), jet kinetic power from \"cavity\" power and bulk Lorentz factor for parsec-scale radio emission, and studied the distributions of these parameters and relations between them. Our main results are as follows. (i) After excluding beaming effect and redshift effect, intrinsic $\\gamma$-ray luminosity with broad line luminosit"},"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":"1404.3556","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-04-14T12:41:37Z","cross_cats_sorted":[],"title_canon_sha256":"94341497f2f711e64caa2a93143214c51db22c40fc69efedfa572b40f06d6a05","abstract_canon_sha256":"29ea7bda2949c5110e0fc57dda5b88ba00983ab1bc7e46e9d011e6f6aa375400"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:34.982571Z","signature_b64":"Y1y19VOpbUjGfPdDJ7LAO3Uc7YcNEgn5p1H6IqpXqYmAQpUOxnjHSQmVfGHEAMIkqE6ZV0LJ3BxFKgjefwZ6Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a27efe51ee88448b030bb6433c1132a1c1a1bf684b26a5e4afd5fe63323deb99","last_reissued_at":"2026-05-18T01:43:34.982024Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:34.982024Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Intrinsic $\\gamma$-ray luminosity, black hole mass, jet and accretion in Fermi blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Dingrong Xiong, Xiong Zhang","submitted_at":"2014-04-14T12:41:37Z","abstract_excerpt":"We have analyzed a large sample of clean blazars detected by Fermi Large Area Telescope (LAT). Using literature and calculation, we obtained intrinsic $\\gamma$-ray luminosity excluding beaming effect, black hole mass, broad-line luminosity (used as a proxy for disk luminosity), jet kinetic power from \"cavity\" power and bulk Lorentz factor for parsec-scale radio emission, and studied the distributions of these parameters and relations between them. Our main results are as follows. (i) After excluding beaming effect and redshift effect, intrinsic $\\gamma$-ray luminosity with broad line luminosit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.3556","kind":"arxiv","version":2},"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":"1404.3556","created_at":"2026-05-18T01:43:34.982116+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.3556v2","created_at":"2026-05-18T01:43:34.982116+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.3556","created_at":"2026-05-18T01:43:34.982116+00:00"},{"alias_kind":"pith_short_12","alias_value":"UJ7P4UPORBCI","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_16","alias_value":"UJ7P4UPORBCIWAYL","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_8","alias_value":"UJ7P4UPO","created_at":"2026-05-18T12:28:52.271510+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/UJ7P4UPORBCIWAYLWZBTYEJSUH","json":"https://pith.science/pith/UJ7P4UPORBCIWAYLWZBTYEJSUH.json","graph_json":"https://pith.science/api/pith-number/UJ7P4UPORBCIWAYLWZBTYEJSUH/graph.json","events_json":"https://pith.science/api/pith-number/UJ7P4UPORBCIWAYLWZBTYEJSUH/events.json","paper":"https://pith.science/paper/UJ7P4UPO"},"agent_actions":{"view_html":"https://pith.science/pith/UJ7P4UPORBCIWAYLWZBTYEJSUH","download_json":"https://pith.science/pith/UJ7P4UPORBCIWAYLWZBTYEJSUH.json","view_paper":"https://pith.science/paper/UJ7P4UPO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.3556&json=true","fetch_graph":"https://pith.science/api/pith-number/UJ7P4UPORBCIWAYLWZBTYEJSUH/graph.json","fetch_events":"https://pith.science/api/pith-number/UJ7P4UPORBCIWAYLWZBTYEJSUH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UJ7P4UPORBCIWAYLWZBTYEJSUH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UJ7P4UPORBCIWAYLWZBTYEJSUH/action/storage_attestation","attest_author":"https://pith.science/pith/UJ7P4UPORBCIWAYLWZBTYEJSUH/action/author_attestation","sign_citation":"https://pith.science/pith/UJ7P4UPORBCIWAYLWZBTYEJSUH/action/citation_signature","submit_replication":"https://pith.science/pith/UJ7P4UPORBCIWAYLWZBTYEJSUH/action/replication_record"}},"created_at":"2026-05-18T01:43:34.982116+00:00","updated_at":"2026-05-18T01:43:34.982116+00:00"}