{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:HFMNYDYQIXOMZCHTBF2OIT3TR2","short_pith_number":"pith:HFMNYDYQ","schema_version":"1.0","canonical_sha256":"3958dc0f1045dccc88f30974e44f738e91408a8a6e943f2a2b528161d83e920f","source":{"kind":"arxiv","id":"2605.22336","version":1},"attestation_state":"computed","paper":{"title":"Seyfert galaxy targets for KM3NeT neutrino telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.Neronov, D.Savchenko, M.Poleshchuk","submitted_at":"2026-05-21T11:24:07Z","abstract_excerpt":"Neutrino signal from a population of Seyfert galaxies has been detected by IceCube neutrino telescope in the muon neutrino channel that has sensitivity mostly to the Northern Hemisphere sources. This detection can be verified by KM3NeT telescope that has sensitivity also in the Southern Hemisphere. We define a catalog of Seyfert galaxies that are expected to be detectable with KM3NeT, assuming that the neutrino luminosity scales with the intrinsic hard X-ray luminosity of the sources. We find that four sources: NGC 1068, NGC 4151, NGC 4945 and Circinus galaxy, are detectable by KM3NeT, if thei"},"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":"2605.22336","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-05-21T11:24:07Z","cross_cats_sorted":[],"title_canon_sha256":"1c0ce347a5b4d34e8c46903f32cc801bc360039d415542602ab7c49e5c8645af","abstract_canon_sha256":"9dc8242ea23417805e3fa82ee355725d28e487fc54a65d90fad0eee35f5b7d7a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-22T01:04:38.336605Z","signature_b64":"RlttUuKx5di2Os7DvGRmuwnO2MK4CvSJmDk+SjxYLj2RYXQ2EijL8yRxsP13fV5cC3vobqBMEvf6E9mbZMlrDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3958dc0f1045dccc88f30974e44f738e91408a8a6e943f2a2b528161d83e920f","last_reissued_at":"2026-05-22T01:04:38.336008Z","signature_status":"signed_v1","first_computed_at":"2026-05-22T01:04:38.336008Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Seyfert galaxy targets for KM3NeT neutrino telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.Neronov, D.Savchenko, M.Poleshchuk","submitted_at":"2026-05-21T11:24:07Z","abstract_excerpt":"Neutrino signal from a population of Seyfert galaxies has been detected by IceCube neutrino telescope in the muon neutrino channel that has sensitivity mostly to the Northern Hemisphere sources. This detection can be verified by KM3NeT telescope that has sensitivity also in the Southern Hemisphere. We define a catalog of Seyfert galaxies that are expected to be detectable with KM3NeT, assuming that the neutrino luminosity scales with the intrinsic hard X-ray luminosity of the sources. We find that four sources: NGC 1068, NGC 4151, NGC 4945 and Circinus galaxy, are detectable by KM3NeT, if thei"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2605.22336","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2605.22336/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2605.22336","created_at":"2026-05-22T01:04:38.336103+00:00"},{"alias_kind":"arxiv_version","alias_value":"2605.22336v1","created_at":"2026-05-22T01:04:38.336103+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.22336","created_at":"2026-05-22T01:04:38.336103+00:00"},{"alias_kind":"pith_short_12","alias_value":"HFMNYDYQIXOM","created_at":"2026-05-22T01:04:38.336103+00:00"},{"alias_kind":"pith_short_16","alias_value":"HFMNYDYQIXOMZCHT","created_at":"2026-05-22T01:04:38.336103+00:00"},{"alias_kind":"pith_short_8","alias_value":"HFMNYDYQ","created_at":"2026-05-22T01:04:38.336103+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/HFMNYDYQIXOMZCHTBF2OIT3TR2","json":"https://pith.science/pith/HFMNYDYQIXOMZCHTBF2OIT3TR2.json","graph_json":"https://pith.science/api/pith-number/HFMNYDYQIXOMZCHTBF2OIT3TR2/graph.json","events_json":"https://pith.science/api/pith-number/HFMNYDYQIXOMZCHTBF2OIT3TR2/events.json","paper":"https://pith.science/paper/HFMNYDYQ"},"agent_actions":{"view_html":"https://pith.science/pith/HFMNYDYQIXOMZCHTBF2OIT3TR2","download_json":"https://pith.science/pith/HFMNYDYQIXOMZCHTBF2OIT3TR2.json","view_paper":"https://pith.science/paper/HFMNYDYQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2605.22336&json=true","fetch_graph":"https://pith.science/api/pith-number/HFMNYDYQIXOMZCHTBF2OIT3TR2/graph.json","fetch_events":"https://pith.science/api/pith-number/HFMNYDYQIXOMZCHTBF2OIT3TR2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HFMNYDYQIXOMZCHTBF2OIT3TR2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HFMNYDYQIXOMZCHTBF2OIT3TR2/action/storage_attestation","attest_author":"https://pith.science/pith/HFMNYDYQIXOMZCHTBF2OIT3TR2/action/author_attestation","sign_citation":"https://pith.science/pith/HFMNYDYQIXOMZCHTBF2OIT3TR2/action/citation_signature","submit_replication":"https://pith.science/pith/HFMNYDYQIXOMZCHTBF2OIT3TR2/action/replication_record"}},"created_at":"2026-05-22T01:04:38.336103+00:00","updated_at":"2026-05-22T01:04:38.336103+00:00"}