{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:OPD3Q6TB56LLVTOC4L6WWJYYSA","short_pith_number":"pith:OPD3Q6TB","schema_version":"1.0","canonical_sha256":"73c7b87a61ef96bacdc2e2fd6b2718900355c6d504977934d8991f973377a608","source":{"kind":"arxiv","id":"1607.04041","version":2},"attestation_state":"computed","paper":{"title":"A flat spectrum candidate for a track-type high energy neutrino emission event, the case of blazar PKS 0723-008","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"E. Kun, L. \\'A. Gergely, P. L. Biermann","submitted_at":"2016-07-14T09:08:36Z","abstract_excerpt":"By cross-correlating both the Parkes Catalogue and the Second Planck Catalogue of Compact Sources with the arrival direction of the track-type neutrinos detected by the IceCube Neutrino Observatory, we find the flat-spectrum blazar PKS 0723-008 as a good candidate for the high-energy neutrino event 5 (ID5). Apart from its coordinates matching those of ID5, PKS 0723-008 exhibits further interesting radio properties. Its spectrum is flat up to high Planck frequencies, and it produced a fivefold-increased radio flux density through the last decade. Based upon these radio properties we propose a s"},"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":"1607.04041","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-07-14T09:08:36Z","cross_cats_sorted":[],"title_canon_sha256":"310751abde34253e430350aa564f5a166e2ec5c14fa1857beaab3a6795b4f2e9","abstract_canon_sha256":"0f79b8de90b306589ee37ff3c93556d7ff73688e475052cff00fc2bbebebfc79"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:53:33.841059Z","signature_b64":"jnCJTsKf0AK/zVspKsTHq3MZImSyMOhUqvLT+bvM4ubaD9UdXmlG6TJCYA8Bymji+cuQgTcJZLl0rrTUb3gOAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"73c7b87a61ef96bacdc2e2fd6b2718900355c6d504977934d8991f973377a608","last_reissued_at":"2026-05-18T00:53:33.840539Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:53:33.840539Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A flat spectrum candidate for a track-type high energy neutrino emission event, the case of blazar PKS 0723-008","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"E. Kun, L. \\'A. Gergely, P. L. Biermann","submitted_at":"2016-07-14T09:08:36Z","abstract_excerpt":"By cross-correlating both the Parkes Catalogue and the Second Planck Catalogue of Compact Sources with the arrival direction of the track-type neutrinos detected by the IceCube Neutrino Observatory, we find the flat-spectrum blazar PKS 0723-008 as a good candidate for the high-energy neutrino event 5 (ID5). Apart from its coordinates matching those of ID5, PKS 0723-008 exhibits further interesting radio properties. Its spectrum is flat up to high Planck frequencies, and it produced a fivefold-increased radio flux density through the last decade. Based upon these radio properties we propose a s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.04041","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":"1607.04041","created_at":"2026-05-18T00:53:33.840625+00:00"},{"alias_kind":"arxiv_version","alias_value":"1607.04041v2","created_at":"2026-05-18T00:53:33.840625+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.04041","created_at":"2026-05-18T00:53:33.840625+00:00"},{"alias_kind":"pith_short_12","alias_value":"OPD3Q6TB56LL","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_16","alias_value":"OPD3Q6TB56LLVTOC","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_8","alias_value":"OPD3Q6TB","created_at":"2026-05-18T12:30:36.002864+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/OPD3Q6TB56LLVTOC4L6WWJYYSA","json":"https://pith.science/pith/OPD3Q6TB56LLVTOC4L6WWJYYSA.json","graph_json":"https://pith.science/api/pith-number/OPD3Q6TB56LLVTOC4L6WWJYYSA/graph.json","events_json":"https://pith.science/api/pith-number/OPD3Q6TB56LLVTOC4L6WWJYYSA/events.json","paper":"https://pith.science/paper/OPD3Q6TB"},"agent_actions":{"view_html":"https://pith.science/pith/OPD3Q6TB56LLVTOC4L6WWJYYSA","download_json":"https://pith.science/pith/OPD3Q6TB56LLVTOC4L6WWJYYSA.json","view_paper":"https://pith.science/paper/OPD3Q6TB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1607.04041&json=true","fetch_graph":"https://pith.science/api/pith-number/OPD3Q6TB56LLVTOC4L6WWJYYSA/graph.json","fetch_events":"https://pith.science/api/pith-number/OPD3Q6TB56LLVTOC4L6WWJYYSA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OPD3Q6TB56LLVTOC4L6WWJYYSA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OPD3Q6TB56LLVTOC4L6WWJYYSA/action/storage_attestation","attest_author":"https://pith.science/pith/OPD3Q6TB56LLVTOC4L6WWJYYSA/action/author_attestation","sign_citation":"https://pith.science/pith/OPD3Q6TB56LLVTOC4L6WWJYYSA/action/citation_signature","submit_replication":"https://pith.science/pith/OPD3Q6TB56LLVTOC4L6WWJYYSA/action/replication_record"}},"created_at":"2026-05-18T00:53:33.840625+00:00","updated_at":"2026-05-18T00:53:33.840625+00:00"}