{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:YOUHB47QJ4V32DVBO3SZOG5E5A","short_pith_number":"pith:YOUHB47Q","schema_version":"1.0","canonical_sha256":"c3a870f3f04f2bbd0ea176e5971ba4e8079c0321a19c9e17f6108084efe8b634","source":{"kind":"arxiv","id":"2307.03259","version":1},"attestation_state":"computed","paper":{"title":"On the Neutrino and Gamma-Ray Emission from NGC 1068","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Carlos Blanco, Dan Hooper, Elena Pinetti, Tim Linden","submitted_at":"2023-07-06T19:35:53Z","abstract_excerpt":"IceCube has recently reported the detection of $\\sim 1-10 \\,{\\rm TeV}$ neutrinos from the nearby active galaxy, NGC 1068. The lack of TeV-scale emission from this source suggests that these neutrinos are generated in the dense corona that surrounds NGC 1068's supermassive black hole. In this paper, we present a physical model for this source, including the processes of pair production, pion production, synchrotron, and inverse Compton scattering. We have also performed a new analysis of Fermi-LAT data from the direction of NGC 1068, finding that the gamma-ray emission from this source is very "},"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":"2307.03259","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-07-06T19:35:53Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"cf6f0afaa430c76087daaa82c3d3cd909a7e1aec7e3e827544bb9da2791cbafb","abstract_canon_sha256":"579fd46fd69244df69b8b3aae452a813eb85cad7ef7ded759583ffb03b24c6da"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:28:40.006492Z","signature_b64":"ynBrtdRyPf3aH3AQXGhZ7fiCrTnIDUgTIXCvxKjqdoFoTqf3GOf/BTlsqTY7PM64Tg/x36b6X75eoAk3w8aUDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c3a870f3f04f2bbd0ea176e5971ba4e8079c0321a19c9e17f6108084efe8b634","last_reissued_at":"2026-07-05T06:28:40.005943Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:28:40.005943Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the Neutrino and Gamma-Ray Emission from NGC 1068","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Carlos Blanco, Dan Hooper, Elena Pinetti, Tim Linden","submitted_at":"2023-07-06T19:35:53Z","abstract_excerpt":"IceCube has recently reported the detection of $\\sim 1-10 \\,{\\rm TeV}$ neutrinos from the nearby active galaxy, NGC 1068. The lack of TeV-scale emission from this source suggests that these neutrinos are generated in the dense corona that surrounds NGC 1068's supermassive black hole. In this paper, we present a physical model for this source, including the processes of pair production, pion production, synchrotron, and inverse Compton scattering. We have also performed a new analysis of Fermi-LAT data from the direction of NGC 1068, finding that the gamma-ray emission from this source is very "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2307.03259","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/2307.03259/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":"2307.03259","created_at":"2026-07-05T06:28:40.006003+00:00"},{"alias_kind":"arxiv_version","alias_value":"2307.03259v1","created_at":"2026-07-05T06:28:40.006003+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2307.03259","created_at":"2026-07-05T06:28:40.006003+00:00"},{"alias_kind":"pith_short_12","alias_value":"YOUHB47QJ4V3","created_at":"2026-07-05T06:28:40.006003+00:00"},{"alias_kind":"pith_short_16","alias_value":"YOUHB47QJ4V32DVB","created_at":"2026-07-05T06:28:40.006003+00:00"},{"alias_kind":"pith_short_8","alias_value":"YOUHB47Q","created_at":"2026-07-05T06:28:40.006003+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2508.11891","citing_title":"High-Energy Neutrinos from Cosmic-Ray Scatterings with Supernova Neutrinos","ref_index":15,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YOUHB47QJ4V32DVBO3SZOG5E5A","json":"https://pith.science/pith/YOUHB47QJ4V32DVBO3SZOG5E5A.json","graph_json":"https://pith.science/api/pith-number/YOUHB47QJ4V32DVBO3SZOG5E5A/graph.json","events_json":"https://pith.science/api/pith-number/YOUHB47QJ4V32DVBO3SZOG5E5A/events.json","paper":"https://pith.science/paper/YOUHB47Q"},"agent_actions":{"view_html":"https://pith.science/pith/YOUHB47QJ4V32DVBO3SZOG5E5A","download_json":"https://pith.science/pith/YOUHB47QJ4V32DVBO3SZOG5E5A.json","view_paper":"https://pith.science/paper/YOUHB47Q","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2307.03259&json=true","fetch_graph":"https://pith.science/api/pith-number/YOUHB47QJ4V32DVBO3SZOG5E5A/graph.json","fetch_events":"https://pith.science/api/pith-number/YOUHB47QJ4V32DVBO3SZOG5E5A/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YOUHB47QJ4V32DVBO3SZOG5E5A/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YOUHB47QJ4V32DVBO3SZOG5E5A/action/storage_attestation","attest_author":"https://pith.science/pith/YOUHB47QJ4V32DVBO3SZOG5E5A/action/author_attestation","sign_citation":"https://pith.science/pith/YOUHB47QJ4V32DVBO3SZOG5E5A/action/citation_signature","submit_replication":"https://pith.science/pith/YOUHB47QJ4V32DVBO3SZOG5E5A/action/replication_record"}},"created_at":"2026-07-05T06:28:40.006003+00:00","updated_at":"2026-07-05T06:28:40.006003+00:00"}