{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:6H6VQE4DOW2DRYJJRLBU57HGHB","short_pith_number":"pith:6H6VQE4D","schema_version":"1.0","canonical_sha256":"f1fd58138375b438e1298ac34efce638582abbbc8b31b8e95579657e110e2c2b","source":{"kind":"arxiv","id":"1701.08781","version":1},"attestation_state":"computed","paper":{"title":"Unveiling slim accretion disc in AGN through X-ray and Infrared observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Chen Hu, Hagai Netzer, Jian-Min Wang, Jin-Ming Bai, Luis C. Ho, N\\'uria Castell\\'o-Mor, Pu Du, Shai Kaspi, Wei-Hao Bian, Ye-Fei Yuan","submitted_at":"2017-01-30T19:01:25Z","abstract_excerpt":"In this work, which is a continuation of Castell\\'o-Mor et al. (2016), we present new X-ray and infrared (IR) data for a sample of active galactic nuclei (AGN) covering a wide range in Eddington ratio over a small luminosity range. In particular, we rigorously explore the dependence of the optical-to-X-ray spectral index $\\alpha_{OX}$ and the IR-to-optical spectral index on the dimensionless accretion rate, $\\dot{\\mathcal{M}}=\\dot{m}/\\eta$ where $\\dot{m}=L_{AGN}/L_{Edd}$ and $\\eta$ is the mass-to-radiation conversion efficiency, in low and high accretion rate sources. We find that the SED of t"},"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":"1701.08781","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-01-30T19:01:25Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"6a7c69d834c27817dabdf50213264ceb74f00d36cc9e4912e35e5c3261ec0a22","abstract_canon_sha256":"a3a970e1c3ce7d7c942765bd50ee86dfcacd653ed82c0cbb6861ef6915804ef7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:51:39.202790Z","signature_b64":"HZ1Czb4AvihTJIeGmu7xeNMSrJBmpYGREPDQTqlzGFZRA+hx4oKX/qX012HVm4TBdbfo0HvAHZ7yebOWQLLqAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f1fd58138375b438e1298ac34efce638582abbbc8b31b8e95579657e110e2c2b","last_reissued_at":"2026-05-18T00:51:39.202257Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:51:39.202257Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Unveiling slim accretion disc in AGN through X-ray and Infrared observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Chen Hu, Hagai Netzer, Jian-Min Wang, Jin-Ming Bai, Luis C. Ho, N\\'uria Castell\\'o-Mor, Pu Du, Shai Kaspi, Wei-Hao Bian, Ye-Fei Yuan","submitted_at":"2017-01-30T19:01:25Z","abstract_excerpt":"In this work, which is a continuation of Castell\\'o-Mor et al. (2016), we present new X-ray and infrared (IR) data for a sample of active galactic nuclei (AGN) covering a wide range in Eddington ratio over a small luminosity range. In particular, we rigorously explore the dependence of the optical-to-X-ray spectral index $\\alpha_{OX}$ and the IR-to-optical spectral index on the dimensionless accretion rate, $\\dot{\\mathcal{M}}=\\dot{m}/\\eta$ where $\\dot{m}=L_{AGN}/L_{Edd}$ and $\\eta$ is the mass-to-radiation conversion efficiency, in low and high accretion rate sources. We find that the SED of t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.08781","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":"1701.08781","created_at":"2026-05-18T00:51:39.202347+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.08781v1","created_at":"2026-05-18T00:51:39.202347+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.08781","created_at":"2026-05-18T00:51:39.202347+00:00"},{"alias_kind":"pith_short_12","alias_value":"6H6VQE4DOW2D","created_at":"2026-05-18T12:31:03.183658+00:00"},{"alias_kind":"pith_short_16","alias_value":"6H6VQE4DOW2DRYJJ","created_at":"2026-05-18T12:31:03.183658+00:00"},{"alias_kind":"pith_short_8","alias_value":"6H6VQE4D","created_at":"2026-05-18T12:31:03.183658+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/6H6VQE4DOW2DRYJJRLBU57HGHB","json":"https://pith.science/pith/6H6VQE4DOW2DRYJJRLBU57HGHB.json","graph_json":"https://pith.science/api/pith-number/6H6VQE4DOW2DRYJJRLBU57HGHB/graph.json","events_json":"https://pith.science/api/pith-number/6H6VQE4DOW2DRYJJRLBU57HGHB/events.json","paper":"https://pith.science/paper/6H6VQE4D"},"agent_actions":{"view_html":"https://pith.science/pith/6H6VQE4DOW2DRYJJRLBU57HGHB","download_json":"https://pith.science/pith/6H6VQE4DOW2DRYJJRLBU57HGHB.json","view_paper":"https://pith.science/paper/6H6VQE4D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.08781&json=true","fetch_graph":"https://pith.science/api/pith-number/6H6VQE4DOW2DRYJJRLBU57HGHB/graph.json","fetch_events":"https://pith.science/api/pith-number/6H6VQE4DOW2DRYJJRLBU57HGHB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6H6VQE4DOW2DRYJJRLBU57HGHB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6H6VQE4DOW2DRYJJRLBU57HGHB/action/storage_attestation","attest_author":"https://pith.science/pith/6H6VQE4DOW2DRYJJRLBU57HGHB/action/author_attestation","sign_citation":"https://pith.science/pith/6H6VQE4DOW2DRYJJRLBU57HGHB/action/citation_signature","submit_replication":"https://pith.science/pith/6H6VQE4DOW2DRYJJRLBU57HGHB/action/replication_record"}},"created_at":"2026-05-18T00:51:39.202347+00:00","updated_at":"2026-05-18T00:51:39.202347+00:00"}