{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:U55VPE5QKD6BLKID2LCZXHNNHI","short_pith_number":"pith:U55VPE5Q","schema_version":"1.0","canonical_sha256":"a77b5793b050fc15a903d2c59b9dad3a31d0dfa9d08b32a301a478a76d562e83","source":{"kind":"arxiv","id":"1909.01993","version":2},"attestation_state":"computed","paper":{"title":"Implications of a proton blazar inspired model on correlated observations of neutrinos with gamma-ray flaring blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Arunava Bhadra, Debasish Majumdar, Madhurima Pandey, Prabir Banik","submitted_at":"2019-09-04T15:43:29Z","abstract_excerpt":"Recent detection of the neutrino events IceCube-170922A, 13 muon-neutrino events observed in 2014-2015 and IceCube-141209A by IceCube observatory from the Blazars, namely TXS 0506+056, PKS 0502+049/TXS 0506+056 and GB6 J1040+0617 respectively in the state of enhanced gamma-ray emission, indicates the acceleration of cosmic rays in the blazar jets. The photo-meson ($p\\gamma$) interaction cannot explain the IceCube observations of 13 neutrino events. The non-detection of broadline emission in the optical spectra of the IceCube blazars, however, question the hadronuclear (pp) interaction interpre"},"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":"1909.01993","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-09-04T15:43:29Z","cross_cats_sorted":[],"title_canon_sha256":"b1c92c3cde0f387634012a0b8251204b20499f3e5275b426e64fd74128dcc1f5","abstract_canon_sha256":"988093709b746dc9561e82c0cbede9257ec0c321786455799ab7413b2ca92716"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:53:40.982211Z","signature_b64":"iwAHgGqOHq+a1AGJ5NhbWaTyR3wDdk0c7BgVqMSuLpkMaDU79E7hkkav6SZ6NL5DfMamXz1JGQ14od9M7sOYBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a77b5793b050fc15a903d2c59b9dad3a31d0dfa9d08b32a301a478a76d562e83","last_reissued_at":"2026-07-05T00:53:40.981780Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:53:40.981780Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Implications of a proton blazar inspired model on correlated observations of neutrinos with gamma-ray flaring blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Arunava Bhadra, Debasish Majumdar, Madhurima Pandey, Prabir Banik","submitted_at":"2019-09-04T15:43:29Z","abstract_excerpt":"Recent detection of the neutrino events IceCube-170922A, 13 muon-neutrino events observed in 2014-2015 and IceCube-141209A by IceCube observatory from the Blazars, namely TXS 0506+056, PKS 0502+049/TXS 0506+056 and GB6 J1040+0617 respectively in the state of enhanced gamma-ray emission, indicates the acceleration of cosmic rays in the blazar jets. The photo-meson ($p\\gamma$) interaction cannot explain the IceCube observations of 13 neutrino events. The non-detection of broadline emission in the optical spectra of the IceCube blazars, however, question the hadronuclear (pp) interaction interpre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1909.01993","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1909.01993/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":"1909.01993","created_at":"2026-07-05T00:53:40.981839+00:00"},{"alias_kind":"arxiv_version","alias_value":"1909.01993v2","created_at":"2026-07-05T00:53:40.981839+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1909.01993","created_at":"2026-07-05T00:53:40.981839+00:00"},{"alias_kind":"pith_short_12","alias_value":"U55VPE5QKD6B","created_at":"2026-07-05T00:53:40.981839+00:00"},{"alias_kind":"pith_short_16","alias_value":"U55VPE5QKD6BLKID","created_at":"2026-07-05T00:53:40.981839+00:00"},{"alias_kind":"pith_short_8","alias_value":"U55VPE5Q","created_at":"2026-07-05T00:53:40.981839+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.23726","citing_title":"A Unified Explanation of Gamma-Ray and Neutrino Spectra from Astrophysical Sources Based on the Gluon Condensation Model","ref_index":33,"is_internal_anchor":false},{"citing_arxiv_id":"2604.23726","citing_title":"A Unified Explanation of Gamma-Ray and Neutrino Spectra from Astrophysical Sources Based on the Gluon Condensation Model","ref_index":33,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/U55VPE5QKD6BLKID2LCZXHNNHI","json":"https://pith.science/pith/U55VPE5QKD6BLKID2LCZXHNNHI.json","graph_json":"https://pith.science/api/pith-number/U55VPE5QKD6BLKID2LCZXHNNHI/graph.json","events_json":"https://pith.science/api/pith-number/U55VPE5QKD6BLKID2LCZXHNNHI/events.json","paper":"https://pith.science/paper/U55VPE5Q"},"agent_actions":{"view_html":"https://pith.science/pith/U55VPE5QKD6BLKID2LCZXHNNHI","download_json":"https://pith.science/pith/U55VPE5QKD6BLKID2LCZXHNNHI.json","view_paper":"https://pith.science/paper/U55VPE5Q","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1909.01993&json=true","fetch_graph":"https://pith.science/api/pith-number/U55VPE5QKD6BLKID2LCZXHNNHI/graph.json","fetch_events":"https://pith.science/api/pith-number/U55VPE5QKD6BLKID2LCZXHNNHI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/U55VPE5QKD6BLKID2LCZXHNNHI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/U55VPE5QKD6BLKID2LCZXHNNHI/action/storage_attestation","attest_author":"https://pith.science/pith/U55VPE5QKD6BLKID2LCZXHNNHI/action/author_attestation","sign_citation":"https://pith.science/pith/U55VPE5QKD6BLKID2LCZXHNNHI/action/citation_signature","submit_replication":"https://pith.science/pith/U55VPE5QKD6BLKID2LCZXHNNHI/action/replication_record"}},"created_at":"2026-07-05T00:53:40.981839+00:00","updated_at":"2026-07-05T00:53:40.981839+00:00"}