{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:PLSHOQLZS2FD6TVE5JK5RJUDKN","short_pith_number":"pith:PLSHOQLZ","schema_version":"1.0","canonical_sha256":"7ae4774179968a3f4ea4ea55d8a6835341faee4a247d5d4b8f5b0690b3d19f9c","source":{"kind":"arxiv","id":"1608.00028","version":2},"attestation_state":"computed","paper":{"title":"Obscured flat spectrum radio AGN as sources of high-energy neutrinos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"G. Gentile, G. Maggi, J. Leon Tavares, K.D. de Vries, M. Vereecken, N. van Eijndhoven, O. Scholten, P. Correa, S. Buitink, T. Winchen","submitted_at":"2016-07-29T20:59:37Z","abstract_excerpt":"Active Galactic Nuclei (AGN) are believed to be one of the main source candidates for the high-energy (TeV-PeV) cosmic neutrino flux recently discovered by the IceCube neutrino observatory. Nevertheless, several correlation studies between AGN and the cosmic neutrinos detected by IceCube show no significance. Therefore, in this article we consider a specific sub-class of AGN for which an increased neutrino production is expected. This sub-class contains AGN for which their high-energy jet is pointing toward Earth. Furthermore, we impose the condition that the jet is obscured by gas or dust sur"},"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":"1608.00028","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-07-29T20:59:37Z","cross_cats_sorted":[],"title_canon_sha256":"adde2a1db15049508c3832ca8c0465ad5a84ecc5a0741d07a1bb39974f36e9df","abstract_canon_sha256":"23b10b37ae94505f03cea1b2e1b3218afdba6747e5312bf973138ce1695a87bd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:57:11.324071Z","signature_b64":"nRa96MBU8vbUjZJjLuMb53rDVS0CQAM+A0WW1Rboa7lSsvJNfYHZKvpyhMLXkLAsM7NIrBM3/xUEtjlKJOLMAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7ae4774179968a3f4ea4ea55d8a6835341faee4a247d5d4b8f5b0690b3d19f9c","last_reissued_at":"2026-05-18T00:57:11.323665Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:57:11.323665Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Obscured flat spectrum radio AGN as sources of high-energy neutrinos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"G. Gentile, G. Maggi, J. Leon Tavares, K.D. de Vries, M. Vereecken, N. van Eijndhoven, O. Scholten, P. Correa, S. Buitink, T. Winchen","submitted_at":"2016-07-29T20:59:37Z","abstract_excerpt":"Active Galactic Nuclei (AGN) are believed to be one of the main source candidates for the high-energy (TeV-PeV) cosmic neutrino flux recently discovered by the IceCube neutrino observatory. Nevertheless, several correlation studies between AGN and the cosmic neutrinos detected by IceCube show no significance. Therefore, in this article we consider a specific sub-class of AGN for which an increased neutrino production is expected. This sub-class contains AGN for which their high-energy jet is pointing toward Earth. Furthermore, we impose the condition that the jet is obscured by gas or dust sur"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.00028","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":"1608.00028","created_at":"2026-05-18T00:57:11.323733+00:00"},{"alias_kind":"arxiv_version","alias_value":"1608.00028v2","created_at":"2026-05-18T00:57:11.323733+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1608.00028","created_at":"2026-05-18T00:57:11.323733+00:00"},{"alias_kind":"pith_short_12","alias_value":"PLSHOQLZS2FD","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_16","alias_value":"PLSHOQLZS2FD6TVE","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_8","alias_value":"PLSHOQLZ","created_at":"2026-05-18T12:30:39.010887+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/PLSHOQLZS2FD6TVE5JK5RJUDKN","json":"https://pith.science/pith/PLSHOQLZS2FD6TVE5JK5RJUDKN.json","graph_json":"https://pith.science/api/pith-number/PLSHOQLZS2FD6TVE5JK5RJUDKN/graph.json","events_json":"https://pith.science/api/pith-number/PLSHOQLZS2FD6TVE5JK5RJUDKN/events.json","paper":"https://pith.science/paper/PLSHOQLZ"},"agent_actions":{"view_html":"https://pith.science/pith/PLSHOQLZS2FD6TVE5JK5RJUDKN","download_json":"https://pith.science/pith/PLSHOQLZS2FD6TVE5JK5RJUDKN.json","view_paper":"https://pith.science/paper/PLSHOQLZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1608.00028&json=true","fetch_graph":"https://pith.science/api/pith-number/PLSHOQLZS2FD6TVE5JK5RJUDKN/graph.json","fetch_events":"https://pith.science/api/pith-number/PLSHOQLZS2FD6TVE5JK5RJUDKN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PLSHOQLZS2FD6TVE5JK5RJUDKN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PLSHOQLZS2FD6TVE5JK5RJUDKN/action/storage_attestation","attest_author":"https://pith.science/pith/PLSHOQLZS2FD6TVE5JK5RJUDKN/action/author_attestation","sign_citation":"https://pith.science/pith/PLSHOQLZS2FD6TVE5JK5RJUDKN/action/citation_signature","submit_replication":"https://pith.science/pith/PLSHOQLZS2FD6TVE5JK5RJUDKN/action/replication_record"}},"created_at":"2026-05-18T00:57:11.323733+00:00","updated_at":"2026-05-18T00:57:11.323733+00:00"}