{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:FD6SR5MGDNJM2MZPWZYL7F5K3O","short_pith_number":"pith:FD6SR5MG","schema_version":"1.0","canonical_sha256":"28fd28f5861b52cd332fb670bf97aadb85daa33fde670403d9006c4138823476","source":{"kind":"arxiv","id":"1201.0988","version":1},"attestation_state":"computed","paper":{"title":"Cosmic Ray Studies with the Fermi Gamma-ray Space Telescope Large Area Telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"David J. Thompson, Luca Baldini, Yasunobu Uchiyama","submitted_at":"2012-01-04T20:54:31Z","abstract_excerpt":"The Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope provides both direct and indirect measurements of Galactic cosmic rays (CR). The LAT high-statistics observations of the 7 GeV - 1 TeV electron plus positron spectrum and limits on spatial anisotropy constrain models for this cosmic-ray component. On a Galactic scale, the LAT observations indicate that cosmic- ray sources may be more plentiful in the outer Galaxy than expected or that the scale height of the cosmic-ray diffusive halo is larger than conventional models. Production of cosmic rays in supernova remnants (SNR) is"},"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":"1201.0988","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-01-04T20:54:31Z","cross_cats_sorted":[],"title_canon_sha256":"12f00a60ba47c928fd4f2457828c315b5d96edb703dd7784ec11911f1774ef99","abstract_canon_sha256":"b858b202390ee24a8baa79520b8018369df42d34f9ceb5fc57c1287fc2711827"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:21:26.054627Z","signature_b64":"GImF/93IUgzgeJkbwj3mYMLT+TKApiKS71gzxqpfOfgb+pzLrNC+8+HAmcpTn63WmkkKw523xGLdw3rOy3UDBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"28fd28f5861b52cd332fb670bf97aadb85daa33fde670403d9006c4138823476","last_reissued_at":"2026-05-18T02:21:26.053888Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:21:26.053888Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmic Ray Studies with the Fermi Gamma-ray Space Telescope Large Area Telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"David J. Thompson, Luca Baldini, Yasunobu Uchiyama","submitted_at":"2012-01-04T20:54:31Z","abstract_excerpt":"The Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope provides both direct and indirect measurements of Galactic cosmic rays (CR). The LAT high-statistics observations of the 7 GeV - 1 TeV electron plus positron spectrum and limits on spatial anisotropy constrain models for this cosmic-ray component. On a Galactic scale, the LAT observations indicate that cosmic- ray sources may be more plentiful in the outer Galaxy than expected or that the scale height of the cosmic-ray diffusive halo is larger than conventional models. Production of cosmic rays in supernova remnants (SNR) is"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.0988","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":"1201.0988","created_at":"2026-05-18T02:21:26.054016+00:00"},{"alias_kind":"arxiv_version","alias_value":"1201.0988v1","created_at":"2026-05-18T02:21:26.054016+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.0988","created_at":"2026-05-18T02:21:26.054016+00:00"},{"alias_kind":"pith_short_12","alias_value":"FD6SR5MGDNJM","created_at":"2026-05-18T12:27:06.952714+00:00"},{"alias_kind":"pith_short_16","alias_value":"FD6SR5MGDNJM2MZP","created_at":"2026-05-18T12:27:06.952714+00:00"},{"alias_kind":"pith_short_8","alias_value":"FD6SR5MG","created_at":"2026-05-18T12:27:06.952714+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/FD6SR5MGDNJM2MZPWZYL7F5K3O","json":"https://pith.science/pith/FD6SR5MGDNJM2MZPWZYL7F5K3O.json","graph_json":"https://pith.science/api/pith-number/FD6SR5MGDNJM2MZPWZYL7F5K3O/graph.json","events_json":"https://pith.science/api/pith-number/FD6SR5MGDNJM2MZPWZYL7F5K3O/events.json","paper":"https://pith.science/paper/FD6SR5MG"},"agent_actions":{"view_html":"https://pith.science/pith/FD6SR5MGDNJM2MZPWZYL7F5K3O","download_json":"https://pith.science/pith/FD6SR5MGDNJM2MZPWZYL7F5K3O.json","view_paper":"https://pith.science/paper/FD6SR5MG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1201.0988&json=true","fetch_graph":"https://pith.science/api/pith-number/FD6SR5MGDNJM2MZPWZYL7F5K3O/graph.json","fetch_events":"https://pith.science/api/pith-number/FD6SR5MGDNJM2MZPWZYL7F5K3O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FD6SR5MGDNJM2MZPWZYL7F5K3O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FD6SR5MGDNJM2MZPWZYL7F5K3O/action/storage_attestation","attest_author":"https://pith.science/pith/FD6SR5MGDNJM2MZPWZYL7F5K3O/action/author_attestation","sign_citation":"https://pith.science/pith/FD6SR5MGDNJM2MZPWZYL7F5K3O/action/citation_signature","submit_replication":"https://pith.science/pith/FD6SR5MGDNJM2MZPWZYL7F5K3O/action/replication_record"}},"created_at":"2026-05-18T02:21:26.054016+00:00","updated_at":"2026-05-18T02:21:26.054016+00:00"}