{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:JKDQPVJNTPHYPV4M3UZOUTKPQR","short_pith_number":"pith:JKDQPVJN","schema_version":"1.0","canonical_sha256":"4a8707d52d9bcf87d78cdd32ea4d4f845215539c541255ffa00a2e1863906d19","source":{"kind":"arxiv","id":"1802.09983","version":3},"attestation_state":"computed","paper":{"title":"Multi-messenger gamma-ray counterpart of the IceCube neutrino signal","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"A.Neronov, D.V. Semikoz, M.Kachelriess","submitted_at":"2018-02-27T16:01:07Z","abstract_excerpt":"A signal of high-energy extraterrestrial neutrinos from unknown source(s) was recently discovered by the IceCube experiment. Neutrinos are always produced together with gamma-rays, but the gamma-ray flux from extragalactic sources is suppressed due to attenuation in the intergalactic medium. We report the discovery of a gamma-ray excess at high Galactic latitudes starting at energies 300 GeV in the data of the Fermi telescope. We show that the multi-TeV gamma-ray diffuse emission has spectral characteristics at both low and high Galactic latitudes compatible with those of the IceCube high neut"},"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":"1802.09983","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-02-27T16:01:07Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"adeb98c941ab263e4c6c6a27fc126aa83f97dabcfbb565269481b66b95655435","abstract_canon_sha256":"c11d2096eaf9dfcd58aee3c4a6ad0040caffd71e120ee1d5e1ec37904a07bbf9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:11:06.044546Z","signature_b64":"xWO5+8Xs6+WP/eXh9inf8eNyniOBGneDplhWqLafBhH1sDYyTGOMtcmqP9l4a/pFK3xj26QRdTtbNqjgV58qCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4a8707d52d9bcf87d78cdd32ea4d4f845215539c541255ffa00a2e1863906d19","last_reissued_at":"2026-05-18T00:11:06.043847Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:11:06.043847Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multi-messenger gamma-ray counterpart of the IceCube neutrino signal","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"A.Neronov, D.V. Semikoz, M.Kachelriess","submitted_at":"2018-02-27T16:01:07Z","abstract_excerpt":"A signal of high-energy extraterrestrial neutrinos from unknown source(s) was recently discovered by the IceCube experiment. Neutrinos are always produced together with gamma-rays, but the gamma-ray flux from extragalactic sources is suppressed due to attenuation in the intergalactic medium. We report the discovery of a gamma-ray excess at high Galactic latitudes starting at energies 300 GeV in the data of the Fermi telescope. We show that the multi-TeV gamma-ray diffuse emission has spectral characteristics at both low and high Galactic latitudes compatible with those of the IceCube high neut"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.09983","kind":"arxiv","version":3},"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":"1802.09983","created_at":"2026-05-18T00:11:06.043986+00:00"},{"alias_kind":"arxiv_version","alias_value":"1802.09983v3","created_at":"2026-05-18T00:11:06.043986+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.09983","created_at":"2026-05-18T00:11:06.043986+00:00"},{"alias_kind":"pith_short_12","alias_value":"JKDQPVJNTPHY","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_16","alias_value":"JKDQPVJNTPHYPV4M","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_8","alias_value":"JKDQPVJN","created_at":"2026-05-18T12:32:31.084164+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1907.10893","citing_title":"Carpet results on astrophysical gamma rays above 100 TeV","ref_index":17,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JKDQPVJNTPHYPV4M3UZOUTKPQR","json":"https://pith.science/pith/JKDQPVJNTPHYPV4M3UZOUTKPQR.json","graph_json":"https://pith.science/api/pith-number/JKDQPVJNTPHYPV4M3UZOUTKPQR/graph.json","events_json":"https://pith.science/api/pith-number/JKDQPVJNTPHYPV4M3UZOUTKPQR/events.json","paper":"https://pith.science/paper/JKDQPVJN"},"agent_actions":{"view_html":"https://pith.science/pith/JKDQPVJNTPHYPV4M3UZOUTKPQR","download_json":"https://pith.science/pith/JKDQPVJNTPHYPV4M3UZOUTKPQR.json","view_paper":"https://pith.science/paper/JKDQPVJN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1802.09983&json=true","fetch_graph":"https://pith.science/api/pith-number/JKDQPVJNTPHYPV4M3UZOUTKPQR/graph.json","fetch_events":"https://pith.science/api/pith-number/JKDQPVJNTPHYPV4M3UZOUTKPQR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JKDQPVJNTPHYPV4M3UZOUTKPQR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JKDQPVJNTPHYPV4M3UZOUTKPQR/action/storage_attestation","attest_author":"https://pith.science/pith/JKDQPVJNTPHYPV4M3UZOUTKPQR/action/author_attestation","sign_citation":"https://pith.science/pith/JKDQPVJNTPHYPV4M3UZOUTKPQR/action/citation_signature","submit_replication":"https://pith.science/pith/JKDQPVJNTPHYPV4M3UZOUTKPQR/action/replication_record"}},"created_at":"2026-05-18T00:11:06.043986+00:00","updated_at":"2026-05-18T00:11:06.043986+00:00"}