{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:VNV4EDD4UC5P4ULI5R6D4B34OV","short_pith_number":"pith:VNV4EDD4","schema_version":"1.0","canonical_sha256":"ab6bc20c7ca0bafe5168ec7c3e077c75541328f78c4f7e63bc4be57829af6d16","source":{"kind":"arxiv","id":"1608.07421","version":2},"attestation_state":"computed","paper":{"title":"Fluxes of diffuse gamma rays and neutrinos from cosmic-ray interactions with circumgalactic gas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Oleg Kalashev, Sergey Troitsky","submitted_at":"2016-08-26T11:02:12Z","abstract_excerpt":"The Milky Way is surrounded by a gravitationally bound gas corona extending up to the Galaxy's virial radius. Interactions of cosmic-ray particles with this gas give rise to energetic secondary gamma rays and neutrinos. We present a quantitative analysis of the neutrino and gamma-ray fluxes from the corona of the Milky Way together with a combined contribution of coronae of other galaxies. The high-energy neutrino flux is insufficient to explain the IceCube results, while the contribution to the FERMI-LAT diffuse gamma-ray flux is not negligible."},"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":"1608.07421","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-08-26T11:02:12Z","cross_cats_sorted":[],"title_canon_sha256":"8daf25479ceee6c884e654e74034aa116e9983a27a168ba0b3776d79067d4fef","abstract_canon_sha256":"c39bb36e903feee579b5ad99ec8580ab64f8326d510b4ec8f2d728fc2e21b20b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:03:17.375154Z","signature_b64":"XLHu5uHCTOmoB1qP4lWj4M3ojJB0nG0gM9yp2oWq4BYdmajSOQJ0lfGeQO6cyAcHffIQIX0o4gF75nG05hwADw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ab6bc20c7ca0bafe5168ec7c3e077c75541328f78c4f7e63bc4be57829af6d16","last_reissued_at":"2026-05-18T01:03:17.374352Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:03:17.374352Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fluxes of diffuse gamma rays and neutrinos from cosmic-ray interactions with circumgalactic gas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Oleg Kalashev, Sergey Troitsky","submitted_at":"2016-08-26T11:02:12Z","abstract_excerpt":"The Milky Way is surrounded by a gravitationally bound gas corona extending up to the Galaxy's virial radius. Interactions of cosmic-ray particles with this gas give rise to energetic secondary gamma rays and neutrinos. We present a quantitative analysis of the neutrino and gamma-ray fluxes from the corona of the Milky Way together with a combined contribution of coronae of other galaxies. The high-energy neutrino flux is insufficient to explain the IceCube results, while the contribution to the FERMI-LAT diffuse gamma-ray flux is not negligible."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.07421","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":"1608.07421","created_at":"2026-05-18T01:03:17.374609+00:00"},{"alias_kind":"arxiv_version","alias_value":"1608.07421v2","created_at":"2026-05-18T01:03:17.374609+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1608.07421","created_at":"2026-05-18T01:03:17.374609+00:00"},{"alias_kind":"pith_short_12","alias_value":"VNV4EDD4UC5P","created_at":"2026-05-18T12:30:48.956258+00:00"},{"alias_kind":"pith_short_16","alias_value":"VNV4EDD4UC5P4ULI","created_at":"2026-05-18T12:30:48.956258+00:00"},{"alias_kind":"pith_short_8","alias_value":"VNV4EDD4","created_at":"2026-05-18T12:30:48.956258+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/VNV4EDD4UC5P4ULI5R6D4B34OV","json":"https://pith.science/pith/VNV4EDD4UC5P4ULI5R6D4B34OV.json","graph_json":"https://pith.science/api/pith-number/VNV4EDD4UC5P4ULI5R6D4B34OV/graph.json","events_json":"https://pith.science/api/pith-number/VNV4EDD4UC5P4ULI5R6D4B34OV/events.json","paper":"https://pith.science/paper/VNV4EDD4"},"agent_actions":{"view_html":"https://pith.science/pith/VNV4EDD4UC5P4ULI5R6D4B34OV","download_json":"https://pith.science/pith/VNV4EDD4UC5P4ULI5R6D4B34OV.json","view_paper":"https://pith.science/paper/VNV4EDD4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1608.07421&json=true","fetch_graph":"https://pith.science/api/pith-number/VNV4EDD4UC5P4ULI5R6D4B34OV/graph.json","fetch_events":"https://pith.science/api/pith-number/VNV4EDD4UC5P4ULI5R6D4B34OV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VNV4EDD4UC5P4ULI5R6D4B34OV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VNV4EDD4UC5P4ULI5R6D4B34OV/action/storage_attestation","attest_author":"https://pith.science/pith/VNV4EDD4UC5P4ULI5R6D4B34OV/action/author_attestation","sign_citation":"https://pith.science/pith/VNV4EDD4UC5P4ULI5R6D4B34OV/action/citation_signature","submit_replication":"https://pith.science/pith/VNV4EDD4UC5P4ULI5R6D4B34OV/action/replication_record"}},"created_at":"2026-05-18T01:03:17.374609+00:00","updated_at":"2026-05-18T01:03:17.374609+00:00"}