{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:VQTBVWRBBE4SA3U4DOJ77VWUSR","short_pith_number":"pith:VQTBVWRB","schema_version":"1.0","canonical_sha256":"ac261ada210939206e9c1b93ffd6d4947e8350ee22aaece8ba0dec77fcca2014","source":{"kind":"arxiv","id":"1501.04335","version":2},"attestation_state":"computed","paper":{"title":"Revisiting the relationship between 6 {\\mu}m and 2-10 keV continuum luminosities of AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Alonso-Herrero, A. Blain, A. Caccianiga, A. Hern\\'an-Caballero, E. Rovilos, F. J. Carrera, P. Severgnini, R. Della Ceca, S. Mateos, X. Barcons","submitted_at":"2015-01-18T18:56:49Z","abstract_excerpt":"We have determined the relation between the AGN luminosities at rest-frame 6 {\\mu}m associated to the dusty torus emission and at 2-10 keV energies using a complete, X-ray flux limited sample of 232 AGN drawn from the Bright Ultra-hard XMM-Newton Survey. The objects have intrinsic X-ray luminosities between 10^42 and 10^46 erg/s and redshifts from 0.05 to 2.8. The rest-frame 6 {\\mu}m luminosities were computed using data from the Wide-Field Infrared Survey Explorer and are based on a spectral energy distribution decomposition into AGN and galaxy emission. The best-fit relationship for the full"},"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":"1501.04335","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-01-18T18:56:49Z","cross_cats_sorted":[],"title_canon_sha256":"927213cffc186c805c1253f5674fe61a8aceb046072b9d25db322a3b786f1c56","abstract_canon_sha256":"6b8cd510a651199fd539672cbb1537138f9e91a2856fb10b35829b4e72778436"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:10.376115Z","signature_b64":"cZ+dL/q0W1fbWzsLQt/RIEJaVvtUUPsHFVv1ZpSo0xxoIeDtkknnyxe99CcZqy+WNgtpoTXK+k9hAyd2Tgr7AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ac261ada210939206e9c1b93ffd6d4947e8350ee22aaece8ba0dec77fcca2014","last_reissued_at":"2026-05-18T01:41:10.375413Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:10.375413Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Revisiting the relationship between 6 {\\mu}m and 2-10 keV continuum luminosities of AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Alonso-Herrero, A. Blain, A. Caccianiga, A. Hern\\'an-Caballero, E. Rovilos, F. J. Carrera, P. Severgnini, R. Della Ceca, S. Mateos, X. Barcons","submitted_at":"2015-01-18T18:56:49Z","abstract_excerpt":"We have determined the relation between the AGN luminosities at rest-frame 6 {\\mu}m associated to the dusty torus emission and at 2-10 keV energies using a complete, X-ray flux limited sample of 232 AGN drawn from the Bright Ultra-hard XMM-Newton Survey. The objects have intrinsic X-ray luminosities between 10^42 and 10^46 erg/s and redshifts from 0.05 to 2.8. The rest-frame 6 {\\mu}m luminosities were computed using data from the Wide-Field Infrared Survey Explorer and are based on a spectral energy distribution decomposition into AGN and galaxy emission. The best-fit relationship for the full"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.04335","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":"1501.04335","created_at":"2026-05-18T01:41:10.375527+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.04335v2","created_at":"2026-05-18T01:41:10.375527+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.04335","created_at":"2026-05-18T01:41:10.375527+00:00"},{"alias_kind":"pith_short_12","alias_value":"VQTBVWRBBE4S","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_16","alias_value":"VQTBVWRBBE4SA3U4","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_8","alias_value":"VQTBVWRB","created_at":"2026-05-18T12:29:47.479230+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/VQTBVWRBBE4SA3U4DOJ77VWUSR","json":"https://pith.science/pith/VQTBVWRBBE4SA3U4DOJ77VWUSR.json","graph_json":"https://pith.science/api/pith-number/VQTBVWRBBE4SA3U4DOJ77VWUSR/graph.json","events_json":"https://pith.science/api/pith-number/VQTBVWRBBE4SA3U4DOJ77VWUSR/events.json","paper":"https://pith.science/paper/VQTBVWRB"},"agent_actions":{"view_html":"https://pith.science/pith/VQTBVWRBBE4SA3U4DOJ77VWUSR","download_json":"https://pith.science/pith/VQTBVWRBBE4SA3U4DOJ77VWUSR.json","view_paper":"https://pith.science/paper/VQTBVWRB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.04335&json=true","fetch_graph":"https://pith.science/api/pith-number/VQTBVWRBBE4SA3U4DOJ77VWUSR/graph.json","fetch_events":"https://pith.science/api/pith-number/VQTBVWRBBE4SA3U4DOJ77VWUSR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VQTBVWRBBE4SA3U4DOJ77VWUSR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VQTBVWRBBE4SA3U4DOJ77VWUSR/action/storage_attestation","attest_author":"https://pith.science/pith/VQTBVWRBBE4SA3U4DOJ77VWUSR/action/author_attestation","sign_citation":"https://pith.science/pith/VQTBVWRBBE4SA3U4DOJ77VWUSR/action/citation_signature","submit_replication":"https://pith.science/pith/VQTBVWRBBE4SA3U4DOJ77VWUSR/action/replication_record"}},"created_at":"2026-05-18T01:41:10.375527+00:00","updated_at":"2026-05-18T01:41:10.375527+00:00"}