{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:DCOVWCB5ZYR5BMJ4BSTRAIMCZO","short_pith_number":"pith:DCOVWCB5","schema_version":"1.0","canonical_sha256":"189d5b083dce23d0b13c0ca7102182cb9dba0450080d6c3d236f99d1d3af446e","source":{"kind":"arxiv","id":"2410.07681","version":1},"attestation_state":"computed","paper":{"title":"Cosmic ray detection with the LOFAR radio telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Corstanje, A. Nelles, B. M. Hare, G. Trinh, H. Falcke, J. R. H\\\"orandel, K. Mulrey, K. Terveer, M. Desmet, N. Karastathis, O. Scholten, P. Laub, P. Turekova, S. Bouma, S. Buitink, S. ter Veen, S. Thoudam, T. Huege","submitted_at":"2024-10-10T07:42:49Z","abstract_excerpt":"The LOw Frequency ARray (LOFAR) has successfully measured cosmic rays for over a decade now. With its dense core of antenna fields in the Netherlands, it is an ideal tool for studying the radio emission from extensive air showers in the $10^{16}$ eV to $10^{18.5}$ eV range. Every air shower is measured with a small particle detector array and hundreds of antennas, which sets LOFAR apart from other air shower arrays. We present our current achievements and progress in reconstruction, interpolation, and software development during the final phases of measurement of LOFAR 1.0, before the LOFAR ar"},"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":"2410.07681","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-10-10T07:42:49Z","cross_cats_sorted":[],"title_canon_sha256":"716e24394671666fec7deee49661e5739bd7be606bccb3764cc539eb2d812ea2","abstract_canon_sha256":"b725fd8c5bc7de995b47e777f5a6da064f8007098ff39b6ea0ccd11d59c6ad8b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:18:41.829448Z","signature_b64":"DCiXsR0BURTAFuK1w32lVVY7N63VFYgfX0QuIT0fODJZwLK8t19qH8qjR3qAd84luQu8J0QeCtvMVQQ4CxCzDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"189d5b083dce23d0b13c0ca7102182cb9dba0450080d6c3d236f99d1d3af446e","last_reissued_at":"2026-07-05T09:18:41.828950Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:18:41.828950Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmic ray detection with the LOFAR radio telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Corstanje, A. Nelles, B. M. Hare, G. Trinh, H. Falcke, J. R. H\\\"orandel, K. Mulrey, K. Terveer, M. Desmet, N. Karastathis, O. Scholten, P. Laub, P. Turekova, S. Bouma, S. Buitink, S. ter Veen, S. Thoudam, T. Huege","submitted_at":"2024-10-10T07:42:49Z","abstract_excerpt":"The LOw Frequency ARray (LOFAR) has successfully measured cosmic rays for over a decade now. With its dense core of antenna fields in the Netherlands, it is an ideal tool for studying the radio emission from extensive air showers in the $10^{16}$ eV to $10^{18.5}$ eV range. Every air shower is measured with a small particle detector array and hundreds of antennas, which sets LOFAR apart from other air shower arrays. We present our current achievements and progress in reconstruction, interpolation, and software development during the final phases of measurement of LOFAR 1.0, before the LOFAR ar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.07681","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2410.07681/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":"2410.07681","created_at":"2026-07-05T09:18:41.829007+00:00"},{"alias_kind":"arxiv_version","alias_value":"2410.07681v1","created_at":"2026-07-05T09:18:41.829007+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2410.07681","created_at":"2026-07-05T09:18:41.829007+00:00"},{"alias_kind":"pith_short_12","alias_value":"DCOVWCB5ZYR5","created_at":"2026-07-05T09:18:41.829007+00:00"},{"alias_kind":"pith_short_16","alias_value":"DCOVWCB5ZYR5BMJ4","created_at":"2026-07-05T09:18:41.829007+00:00"},{"alias_kind":"pith_short_8","alias_value":"DCOVWCB5","created_at":"2026-07-05T09:18:41.829007+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.26702","citing_title":"Interferometric Analysis of Air-shower Radio Emission in the Near Field with an Information Field Theory Approach","ref_index":31,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DCOVWCB5ZYR5BMJ4BSTRAIMCZO","json":"https://pith.science/pith/DCOVWCB5ZYR5BMJ4BSTRAIMCZO.json","graph_json":"https://pith.science/api/pith-number/DCOVWCB5ZYR5BMJ4BSTRAIMCZO/graph.json","events_json":"https://pith.science/api/pith-number/DCOVWCB5ZYR5BMJ4BSTRAIMCZO/events.json","paper":"https://pith.science/paper/DCOVWCB5"},"agent_actions":{"view_html":"https://pith.science/pith/DCOVWCB5ZYR5BMJ4BSTRAIMCZO","download_json":"https://pith.science/pith/DCOVWCB5ZYR5BMJ4BSTRAIMCZO.json","view_paper":"https://pith.science/paper/DCOVWCB5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2410.07681&json=true","fetch_graph":"https://pith.science/api/pith-number/DCOVWCB5ZYR5BMJ4BSTRAIMCZO/graph.json","fetch_events":"https://pith.science/api/pith-number/DCOVWCB5ZYR5BMJ4BSTRAIMCZO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DCOVWCB5ZYR5BMJ4BSTRAIMCZO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DCOVWCB5ZYR5BMJ4BSTRAIMCZO/action/storage_attestation","attest_author":"https://pith.science/pith/DCOVWCB5ZYR5BMJ4BSTRAIMCZO/action/author_attestation","sign_citation":"https://pith.science/pith/DCOVWCB5ZYR5BMJ4BSTRAIMCZO/action/citation_signature","submit_replication":"https://pith.science/pith/DCOVWCB5ZYR5BMJ4BSTRAIMCZO/action/replication_record"}},"created_at":"2026-07-05T09:18:41.829007+00:00","updated_at":"2026-07-05T09:18:41.829007+00:00"}