{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:P5H2MMUEHNVACRACMKKDCEX6ZM","short_pith_number":"pith:P5H2MMUE","schema_version":"1.0","canonical_sha256":"7f4fa632843b6a01440262943112fecb0c5a43d982790511fe5ae4308a415227","source":{"kind":"arxiv","id":"0710.1382","version":2},"attestation_state":"computed","paper":{"title":"Global anisotropy of arrival directions of ultra-high-energy cosmic rays: capabilities of space-based detectors","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B.A. Khrenov, O.E. Kalashev, P. Klimov, S. Sharakin, S.V. Troitsky","submitted_at":"2007-10-06T17:50:41Z","abstract_excerpt":"Planned space-based ultra-high-energy cosmic-ray detectors (TUS, JEM-EUSO and S-EUSO) are best suited for searches of global anisotropies in the distribution of arrival directions of cosmic-ray particles because they will be able to observe the full sky with a single instrument. We calculate quantitatively the strength of anisotropies associated with two models of the origin of the highest-energy particles: the extragalactic model (sources follow the distribution of galaxies in the Universe) and the superheavy dark-matter model (sources follow the distribution of dark matter in the Galactic ha"},"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":"0710.1382","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2007-10-06T17:50:41Z","cross_cats_sorted":[],"title_canon_sha256":"13e4bd1e43d23f1d8ae88bce92d15c507673f6e9e50cc33dfe57f63e381aaf1f","abstract_canon_sha256":"457a166617edb514f1d712e2f7055791770bde712a6ad5264360c88515a2941c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:35:24.622470Z","signature_b64":"X2U7ZGm7KtaN30owZmzrEx2RM+l+7sVJxVJrE1Z23+9rUL1HPHQVUk3lwZ5HP5TJfBN3CjXJdTJcQRwtXiAlBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7f4fa632843b6a01440262943112fecb0c5a43d982790511fe5ae4308a415227","last_reissued_at":"2026-05-18T02:35:24.621912Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:35:24.621912Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Global anisotropy of arrival directions of ultra-high-energy cosmic rays: capabilities of space-based detectors","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B.A. Khrenov, O.E. Kalashev, P. Klimov, S. Sharakin, S.V. Troitsky","submitted_at":"2007-10-06T17:50:41Z","abstract_excerpt":"Planned space-based ultra-high-energy cosmic-ray detectors (TUS, JEM-EUSO and S-EUSO) are best suited for searches of global anisotropies in the distribution of arrival directions of cosmic-ray particles because they will be able to observe the full sky with a single instrument. We calculate quantitatively the strength of anisotropies associated with two models of the origin of the highest-energy particles: the extragalactic model (sources follow the distribution of galaxies in the Universe) and the superheavy dark-matter model (sources follow the distribution of dark matter in the Galactic ha"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0710.1382","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":"0710.1382","created_at":"2026-05-18T02:35:24.621981+00:00"},{"alias_kind":"arxiv_version","alias_value":"0710.1382v2","created_at":"2026-05-18T02:35:24.621981+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0710.1382","created_at":"2026-05-18T02:35:24.621981+00:00"},{"alias_kind":"pith_short_12","alias_value":"P5H2MMUEHNVA","created_at":"2026-05-18T12:25:55.427421+00:00"},{"alias_kind":"pith_short_16","alias_value":"P5H2MMUEHNVACRAC","created_at":"2026-05-18T12:25:55.427421+00:00"},{"alias_kind":"pith_short_8","alias_value":"P5H2MMUE","created_at":"2026-05-18T12:25:55.427421+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/P5H2MMUEHNVACRACMKKDCEX6ZM","json":"https://pith.science/pith/P5H2MMUEHNVACRACMKKDCEX6ZM.json","graph_json":"https://pith.science/api/pith-number/P5H2MMUEHNVACRACMKKDCEX6ZM/graph.json","events_json":"https://pith.science/api/pith-number/P5H2MMUEHNVACRACMKKDCEX6ZM/events.json","paper":"https://pith.science/paper/P5H2MMUE"},"agent_actions":{"view_html":"https://pith.science/pith/P5H2MMUEHNVACRACMKKDCEX6ZM","download_json":"https://pith.science/pith/P5H2MMUEHNVACRACMKKDCEX6ZM.json","view_paper":"https://pith.science/paper/P5H2MMUE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0710.1382&json=true","fetch_graph":"https://pith.science/api/pith-number/P5H2MMUEHNVACRACMKKDCEX6ZM/graph.json","fetch_events":"https://pith.science/api/pith-number/P5H2MMUEHNVACRACMKKDCEX6ZM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/P5H2MMUEHNVACRACMKKDCEX6ZM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/P5H2MMUEHNVACRACMKKDCEX6ZM/action/storage_attestation","attest_author":"https://pith.science/pith/P5H2MMUEHNVACRACMKKDCEX6ZM/action/author_attestation","sign_citation":"https://pith.science/pith/P5H2MMUEHNVACRACMKKDCEX6ZM/action/citation_signature","submit_replication":"https://pith.science/pith/P5H2MMUEHNVACRACMKKDCEX6ZM/action/replication_record"}},"created_at":"2026-05-18T02:35:24.621981+00:00","updated_at":"2026-05-18T02:35:24.621981+00:00"}