{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:CULBJEHJ77GYN4BHPKKZLFALBJ","short_pith_number":"pith:CULBJEHJ","schema_version":"1.0","canonical_sha256":"15161490e9ffcd86f0277a9595940b0a4f9e3b5d6e75bd724ed4c0af969b4092","source":{"kind":"arxiv","id":"1703.10398","version":1},"attestation_state":"computed","paper":{"title":"Does the SN rate explain the very high energy cosmic rays in the central 200 pc of our Galaxy?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Lemi\\`ere, L. Jouvin, R. Terrier","submitted_at":"2017-03-30T10:42:48Z","abstract_excerpt":"The H.E.S.S. collaboration revealed the presence of a very high energy (VHE) diffuse emission in the inner 100pc of the Galaxy in close correlation with the Central Molecular Zone (CMZ). Recently, they deduced from this emission a cosmic-ray (CR) over-density in the region with a local peak toward the Galactic Center (GC) and proposed a diffusive scenario with a stationary source at the GC to explain it. However, the high supernovae (SN) rate in the GC must also create a sustained CR injection in the region via the shocks produced at the time of their explosion. Considering typical diffusion c"},"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":"1703.10398","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-03-30T10:42:48Z","cross_cats_sorted":[],"title_canon_sha256":"bb1b524c658d9695a2b56cbd25a2fb95a033b01857aaf502fb6a2f2435ad617b","abstract_canon_sha256":"18f450e287247b289dbd46e8a52ce1bcb7cd12e7575c27db8cdaf94b5213e76a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:47:36.765788Z","signature_b64":"kWYktBmzjlenyV+P0OjydKk7yoMmUP8Jr9B9aFuUFGdXLDG6NZBGhBYTkECPSDr0Il5YgnTPkjvRC18ekKciDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"15161490e9ffcd86f0277a9595940b0a4f9e3b5d6e75bd724ed4c0af969b4092","last_reissued_at":"2026-05-18T00:47:36.765162Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:47:36.765162Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Does the SN rate explain the very high energy cosmic rays in the central 200 pc of our Galaxy?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Lemi\\`ere, L. Jouvin, R. Terrier","submitted_at":"2017-03-30T10:42:48Z","abstract_excerpt":"The H.E.S.S. collaboration revealed the presence of a very high energy (VHE) diffuse emission in the inner 100pc of the Galaxy in close correlation with the Central Molecular Zone (CMZ). Recently, they deduced from this emission a cosmic-ray (CR) over-density in the region with a local peak toward the Galactic Center (GC) and proposed a diffusive scenario with a stationary source at the GC to explain it. However, the high supernovae (SN) rate in the GC must also create a sustained CR injection in the region via the shocks produced at the time of their explosion. Considering typical diffusion c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.10398","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":""},"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":"1703.10398","created_at":"2026-05-18T00:47:36.765259+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.10398v1","created_at":"2026-05-18T00:47:36.765259+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.10398","created_at":"2026-05-18T00:47:36.765259+00:00"},{"alias_kind":"pith_short_12","alias_value":"CULBJEHJ77GY","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_16","alias_value":"CULBJEHJ77GYN4BH","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_8","alias_value":"CULBJEHJ","created_at":"2026-05-18T12:31:10.602751+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/CULBJEHJ77GYN4BHPKKZLFALBJ","json":"https://pith.science/pith/CULBJEHJ77GYN4BHPKKZLFALBJ.json","graph_json":"https://pith.science/api/pith-number/CULBJEHJ77GYN4BHPKKZLFALBJ/graph.json","events_json":"https://pith.science/api/pith-number/CULBJEHJ77GYN4BHPKKZLFALBJ/events.json","paper":"https://pith.science/paper/CULBJEHJ"},"agent_actions":{"view_html":"https://pith.science/pith/CULBJEHJ77GYN4BHPKKZLFALBJ","download_json":"https://pith.science/pith/CULBJEHJ77GYN4BHPKKZLFALBJ.json","view_paper":"https://pith.science/paper/CULBJEHJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.10398&json=true","fetch_graph":"https://pith.science/api/pith-number/CULBJEHJ77GYN4BHPKKZLFALBJ/graph.json","fetch_events":"https://pith.science/api/pith-number/CULBJEHJ77GYN4BHPKKZLFALBJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CULBJEHJ77GYN4BHPKKZLFALBJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CULBJEHJ77GYN4BHPKKZLFALBJ/action/storage_attestation","attest_author":"https://pith.science/pith/CULBJEHJ77GYN4BHPKKZLFALBJ/action/author_attestation","sign_citation":"https://pith.science/pith/CULBJEHJ77GYN4BHPKKZLFALBJ/action/citation_signature","submit_replication":"https://pith.science/pith/CULBJEHJ77GYN4BHPKKZLFALBJ/action/replication_record"}},"created_at":"2026-05-18T00:47:36.765259+00:00","updated_at":"2026-05-18T00:47:36.765259+00:00"}