{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:JORTGOW5PLZCORIPO24GZ3XXLX","short_pith_number":"pith:JORTGOW5","schema_version":"1.0","canonical_sha256":"4ba3333add7af227450f76b86ceef75dc2fdfe15159eb88871165600385f51ea","source":{"kind":"arxiv","id":"2303.08766","version":2},"attestation_state":"computed","paper":{"title":"Modification of the Dipole in Arrival Directions of Ultra-high-energy Cosmic Rays due to the Galactic Magnetic Field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alena Bakalov\\'a, Jakub V\\'icha, Petr Tr\\'avn\\'i\\v{c}ek","submitted_at":"2023-03-15T17:05:02Z","abstract_excerpt":"The direction and magnitude of the dipole anisotropy of ultra-high-energy cosmic rays with energies above 8 EeV observed by the Pierre Auger Observatory indicate their extragalactic origin. The observed dipole on Earth does not necessarily need to correspond to the anisotropy of the extragalactic cosmic-ray flux due to the effects of propagation in the Galactic magnetic field. We estimate the size of these effects via numerical simulations using the CRPropa 3 package. The Jansson-Farrar and Terral-Ferri\\`ere models of the Galactic magnetic field are used to propagate particles from the edge of"},"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":"2303.08766","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-03-15T17:05:02Z","cross_cats_sorted":[],"title_canon_sha256":"82e22a1ca1b95c2204d94040d03ca5cf382cc28c328787c0a17722e05722f403","abstract_canon_sha256":"5751d804de0eacccd64343a099ce1cfe73980100511c8f5a23c852f5404d617d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:43:51.929567Z","signature_b64":"/ytNMI/Uj8m/NpHixFryGRRGbdd0HHACD8+Gj+Quc0a+y+znmRylC3Xw3Shx13MZ28XfLx5wHgzeIGnqCgK2Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4ba3333add7af227450f76b86ceef75dc2fdfe15159eb88871165600385f51ea","last_reissued_at":"2026-07-05T07:43:51.929092Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:43:51.929092Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Modification of the Dipole in Arrival Directions of Ultra-high-energy Cosmic Rays due to the Galactic Magnetic Field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alena Bakalov\\'a, Jakub V\\'icha, Petr Tr\\'avn\\'i\\v{c}ek","submitted_at":"2023-03-15T17:05:02Z","abstract_excerpt":"The direction and magnitude of the dipole anisotropy of ultra-high-energy cosmic rays with energies above 8 EeV observed by the Pierre Auger Observatory indicate their extragalactic origin. The observed dipole on Earth does not necessarily need to correspond to the anisotropy of the extragalactic cosmic-ray flux due to the effects of propagation in the Galactic magnetic field. We estimate the size of these effects via numerical simulations using the CRPropa 3 package. The Jansson-Farrar and Terral-Ferri\\`ere models of the Galactic magnetic field are used to propagate particles from the edge of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2303.08766","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/2303.08766/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":"2303.08766","created_at":"2026-07-05T07:43:51.929149+00:00"},{"alias_kind":"arxiv_version","alias_value":"2303.08766v2","created_at":"2026-07-05T07:43:51.929149+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2303.08766","created_at":"2026-07-05T07:43:51.929149+00:00"},{"alias_kind":"pith_short_12","alias_value":"JORTGOW5PLZC","created_at":"2026-07-05T07:43:51.929149+00:00"},{"alias_kind":"pith_short_16","alias_value":"JORTGOW5PLZCORIP","created_at":"2026-07-05T07:43:51.929149+00:00"},{"alias_kind":"pith_short_8","alias_value":"JORTGOW5","created_at":"2026-07-05T07:43:51.929149+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2502.08747","citing_title":"Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays","ref_index":24,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JORTGOW5PLZCORIPO24GZ3XXLX","json":"https://pith.science/pith/JORTGOW5PLZCORIPO24GZ3XXLX.json","graph_json":"https://pith.science/api/pith-number/JORTGOW5PLZCORIPO24GZ3XXLX/graph.json","events_json":"https://pith.science/api/pith-number/JORTGOW5PLZCORIPO24GZ3XXLX/events.json","paper":"https://pith.science/paper/JORTGOW5"},"agent_actions":{"view_html":"https://pith.science/pith/JORTGOW5PLZCORIPO24GZ3XXLX","download_json":"https://pith.science/pith/JORTGOW5PLZCORIPO24GZ3XXLX.json","view_paper":"https://pith.science/paper/JORTGOW5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2303.08766&json=true","fetch_graph":"https://pith.science/api/pith-number/JORTGOW5PLZCORIPO24GZ3XXLX/graph.json","fetch_events":"https://pith.science/api/pith-number/JORTGOW5PLZCORIPO24GZ3XXLX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JORTGOW5PLZCORIPO24GZ3XXLX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JORTGOW5PLZCORIPO24GZ3XXLX/action/storage_attestation","attest_author":"https://pith.science/pith/JORTGOW5PLZCORIPO24GZ3XXLX/action/author_attestation","sign_citation":"https://pith.science/pith/JORTGOW5PLZCORIPO24GZ3XXLX/action/citation_signature","submit_replication":"https://pith.science/pith/JORTGOW5PLZCORIPO24GZ3XXLX/action/replication_record"}},"created_at":"2026-07-05T07:43:51.929149+00:00","updated_at":"2026-07-05T07:43:51.929149+00:00"}