{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:EBF323TRPSB4GPLGSTM2BMXJHF","short_pith_number":"pith:EBF323TR","schema_version":"1.0","canonical_sha256":"204bbd6e717c83c33d6694d9a0b2e9396dbd892ac5850dac8dcfe1012b314a2f","source":{"kind":"arxiv","id":"2504.18257","version":2},"attestation_state":"computed","paper":{"title":"Reconstruction of inclined extensive air showers using radio signals: from arrival times and amplitudes to direction and energy","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"astro-ph.HE","authors_text":"Aur\\'elien Benoit-L\\'evy, Marion Guelfand, Mat\\'ias Tueros, Olivier Martineau-Huynh, Oscar Macias, Simon Prunet, Valentin Decoene","submitted_at":"2025-04-25T11:02:51Z","abstract_excerpt":"Radio detection is now an established technique for the study of ultra-high-energy (UHE) cosmic rays with energies above $\\sim10^{17}$ eV. The next-generation of radio experiments aims to extend this technique to the observation of UHE earth-skimming neutrinos, which requires the detection of very inclined extensive air showers (EAS). In this article we present a new reconstruction method for the arrival direction and the energy of EAS. It combines a point-source-like description of the radio wavefront with a phenomenological model: the Angular Distribution Function (ADF). The ADF describes th"},"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":"2504.18257","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-04-25T11:02:51Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"a72cafbd21f6738bf5c35fcbfd0f5929c37acc2292bd122caeb91eeb23eeab40","abstract_canon_sha256":"26609e0114e4cc87ceb823245691da33547b1d1d530bfe1203780f4a6a6c5c58"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:01:57.198899Z","signature_b64":"xR/mb0sNQ5gxZse5UctYSCGIpW2NpcI2yh7f1/Xi/4GY1lmsbGrndjxZJ9y1l5azRt/doO+Hk/zH8SZ91eDHDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"204bbd6e717c83c33d6694d9a0b2e9396dbd892ac5850dac8dcfe1012b314a2f","last_reissued_at":"2026-07-05T11:01:57.198389Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:01:57.198389Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Reconstruction of inclined extensive air showers using radio signals: from arrival times and amplitudes to direction and energy","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"astro-ph.HE","authors_text":"Aur\\'elien Benoit-L\\'evy, Marion Guelfand, Mat\\'ias Tueros, Olivier Martineau-Huynh, Oscar Macias, Simon Prunet, Valentin Decoene","submitted_at":"2025-04-25T11:02:51Z","abstract_excerpt":"Radio detection is now an established technique for the study of ultra-high-energy (UHE) cosmic rays with energies above $\\sim10^{17}$ eV. The next-generation of radio experiments aims to extend this technique to the observation of UHE earth-skimming neutrinos, which requires the detection of very inclined extensive air showers (EAS). In this article we present a new reconstruction method for the arrival direction and the energy of EAS. It combines a point-source-like description of the radio wavefront with a phenomenological model: the Angular Distribution Function (ADF). The ADF describes th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2504.18257","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/2504.18257/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":"2504.18257","created_at":"2026-07-05T11:01:57.198449+00:00"},{"alias_kind":"arxiv_version","alias_value":"2504.18257v2","created_at":"2026-07-05T11:01:57.198449+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2504.18257","created_at":"2026-07-05T11:01:57.198449+00:00"},{"alias_kind":"pith_short_12","alias_value":"EBF323TRPSB4","created_at":"2026-07-05T11:01:57.198449+00:00"},{"alias_kind":"pith_short_16","alias_value":"EBF323TRPSB4GPLG","created_at":"2026-07-05T11:01:57.198449+00:00"},{"alias_kind":"pith_short_8","alias_value":"EBF323TR","created_at":"2026-07-05T11:01:57.198449+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.06695","citing_title":"Search for cosmic rays in GRANDProto300","ref_index":14,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EBF323TRPSB4GPLGSTM2BMXJHF","json":"https://pith.science/pith/EBF323TRPSB4GPLGSTM2BMXJHF.json","graph_json":"https://pith.science/api/pith-number/EBF323TRPSB4GPLGSTM2BMXJHF/graph.json","events_json":"https://pith.science/api/pith-number/EBF323TRPSB4GPLGSTM2BMXJHF/events.json","paper":"https://pith.science/paper/EBF323TR"},"agent_actions":{"view_html":"https://pith.science/pith/EBF323TRPSB4GPLGSTM2BMXJHF","download_json":"https://pith.science/pith/EBF323TRPSB4GPLGSTM2BMXJHF.json","view_paper":"https://pith.science/paper/EBF323TR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2504.18257&json=true","fetch_graph":"https://pith.science/api/pith-number/EBF323TRPSB4GPLGSTM2BMXJHF/graph.json","fetch_events":"https://pith.science/api/pith-number/EBF323TRPSB4GPLGSTM2BMXJHF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EBF323TRPSB4GPLGSTM2BMXJHF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EBF323TRPSB4GPLGSTM2BMXJHF/action/storage_attestation","attest_author":"https://pith.science/pith/EBF323TRPSB4GPLGSTM2BMXJHF/action/author_attestation","sign_citation":"https://pith.science/pith/EBF323TRPSB4GPLGSTM2BMXJHF/action/citation_signature","submit_replication":"https://pith.science/pith/EBF323TRPSB4GPLGSTM2BMXJHF/action/replication_record"}},"created_at":"2026-07-05T11:01:57.198449+00:00","updated_at":"2026-07-05T11:01:57.198449+00:00"}