{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:UOGXRCZOSUICIJAYFFNQAPQTZV","short_pith_number":"pith:UOGXRCZO","schema_version":"1.0","canonical_sha256":"a38d788b2e9510242418295b003e13cd75e3836b2b464cd07c29195bf51a2518","source":{"kind":"arxiv","id":"1508.01919","version":1},"attestation_state":"computed","paper":{"title":"The Giant Radio Array for Neutrino Detection","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Chad Finley, Charles Timmermans, Didier Charrier, Foteini Oikonomou, Hongbo Hu, Jianli Zhang, Julia Schmid, Junhua Gu, Ke Fang, Kohta Murase, Krijn D. de Vries, Kumiko Kotera, Nicolas Renault-Tinacci, Olivier Martineau-Huynh, Quanbu Gou, Sijbrand de Jong, Valentin Niess, Xiangping Wu, Yi Zhang, Zhaoyang Feng, Zhen Wang","submitted_at":"2015-08-08T15:45:58Z","abstract_excerpt":"High-energy neutrino astronomy will probe the working of the most violent phenomena in the Universe. The Giant Radio Array for Neutrino Detection (GRAND) project consists of an array of $\\sim10^5$ radio antennas deployed over $\\sim$200000km$^2$ in a mountainous site. It aims at detecting high-energy neutrinos via the measurement of air showers induced by the decay in the atmosphere of $\\tau$ leptons produced by the interaction of the cosmic neutrinos under the Earth surface. Our objective with GRAND is to reach a neutrino sensitivity of $3\\times10^{-11}E^{-2}$GeV$^{-1}$cm$^{-2}$s$^{-1}$sr$^{-1"},"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":"1508.01919","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-08-08T15:45:58Z","cross_cats_sorted":[],"title_canon_sha256":"ed3a9c5f6f415d4dae58578b222cfb78bb75f506482e09334f962583483eb2f7","abstract_canon_sha256":"9ba1f1bdf18c95517c71a73e89a30ee7a8f84d8fd7685ad623664ebba9dfa5e8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:16:18.385213Z","signature_b64":"7gezk++8D1ktSr4LEGlAUt1R9OZyjbD7LNmf65GTJycADVGHJ5okKUO6ahF7Sui5urxSPUwDywj2kC5bCeHyDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a38d788b2e9510242418295b003e13cd75e3836b2b464cd07c29195bf51a2518","last_reissued_at":"2026-05-18T01:16:18.384520Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:16:18.384520Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Giant Radio Array for Neutrino Detection","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Chad Finley, Charles Timmermans, Didier Charrier, Foteini Oikonomou, Hongbo Hu, Jianli Zhang, Julia Schmid, Junhua Gu, Ke Fang, Kohta Murase, Krijn D. de Vries, Kumiko Kotera, Nicolas Renault-Tinacci, Olivier Martineau-Huynh, Quanbu Gou, Sijbrand de Jong, Valentin Niess, Xiangping Wu, Yi Zhang, Zhaoyang Feng, Zhen Wang","submitted_at":"2015-08-08T15:45:58Z","abstract_excerpt":"High-energy neutrino astronomy will probe the working of the most violent phenomena in the Universe. The Giant Radio Array for Neutrino Detection (GRAND) project consists of an array of $\\sim10^5$ radio antennas deployed over $\\sim$200000km$^2$ in a mountainous site. It aims at detecting high-energy neutrinos via the measurement of air showers induced by the decay in the atmosphere of $\\tau$ leptons produced by the interaction of the cosmic neutrinos under the Earth surface. Our objective with GRAND is to reach a neutrino sensitivity of $3\\times10^{-11}E^{-2}$GeV$^{-1}$cm$^{-2}$s$^{-1}$sr$^{-1"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.01919","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":"1508.01919","created_at":"2026-05-18T01:16:18.384639+00:00"},{"alias_kind":"arxiv_version","alias_value":"1508.01919v1","created_at":"2026-05-18T01:16:18.384639+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1508.01919","created_at":"2026-05-18T01:16:18.384639+00:00"},{"alias_kind":"pith_short_12","alias_value":"UOGXRCZOSUIC","created_at":"2026-05-18T12:29:44.643036+00:00"},{"alias_kind":"pith_short_16","alias_value":"UOGXRCZOSUICIJAY","created_at":"2026-05-18T12:29:44.643036+00:00"},{"alias_kind":"pith_short_8","alias_value":"UOGXRCZO","created_at":"2026-05-18T12:29:44.643036+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/UOGXRCZOSUICIJAYFFNQAPQTZV","json":"https://pith.science/pith/UOGXRCZOSUICIJAYFFNQAPQTZV.json","graph_json":"https://pith.science/api/pith-number/UOGXRCZOSUICIJAYFFNQAPQTZV/graph.json","events_json":"https://pith.science/api/pith-number/UOGXRCZOSUICIJAYFFNQAPQTZV/events.json","paper":"https://pith.science/paper/UOGXRCZO"},"agent_actions":{"view_html":"https://pith.science/pith/UOGXRCZOSUICIJAYFFNQAPQTZV","download_json":"https://pith.science/pith/UOGXRCZOSUICIJAYFFNQAPQTZV.json","view_paper":"https://pith.science/paper/UOGXRCZO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1508.01919&json=true","fetch_graph":"https://pith.science/api/pith-number/UOGXRCZOSUICIJAYFFNQAPQTZV/graph.json","fetch_events":"https://pith.science/api/pith-number/UOGXRCZOSUICIJAYFFNQAPQTZV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UOGXRCZOSUICIJAYFFNQAPQTZV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UOGXRCZOSUICIJAYFFNQAPQTZV/action/storage_attestation","attest_author":"https://pith.science/pith/UOGXRCZOSUICIJAYFFNQAPQTZV/action/author_attestation","sign_citation":"https://pith.science/pith/UOGXRCZOSUICIJAYFFNQAPQTZV/action/citation_signature","submit_replication":"https://pith.science/pith/UOGXRCZOSUICIJAYFFNQAPQTZV/action/replication_record"}},"created_at":"2026-05-18T01:16:18.384639+00:00","updated_at":"2026-05-18T01:16:18.384639+00:00"}