{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:KJU644U2CTLN2NEUB5ICZK5RSR","short_pith_number":"pith:KJU644U2","schema_version":"1.0","canonical_sha256":"5269ee729a14d6dd34940f502cabb1947f9d0bcac66f95beea4428df96fd4398","source":{"kind":"arxiv","id":"1404.5285","version":3},"attestation_state":"computed","paper":{"title":"First Constraints on the Ultra-High Energy Neutrino Flux from a Prototype Station of the Askaryan Radio Array","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"A. Connolly, A. Ishihara, A. Karle, A. Laundrie, A. O'Murchadha, ARA Collaboration: P. Allison, A. Shultz, B. Fox, B. Hill, B. Rotter, C. Bora, C.-C. Chen, C. G. Pfendner, C.-J. Li, C. Miki, D. Seckel, D. Z. Besson, E. Hong, G. Nir, G. S. Varner, H. Landsman, H.-Y. Tu, I. Kravchenko, J. Auffenberg, J. J. Beatty, J. Kelley, J. Nam, J. P. Davies, J. Stockham, J. Touart, K. D. Hoffman, K. Hanson, K. Mase, K. Ratzlaff, L.-C. Hu, M. A. DuVernois, M. Richman, M. Stockham, M. Sullivan, M.-Y. Lu, P. Chen, P. Sandstrom, P. W. Gorham, R. Bard, R. J. Nichol, R. Maunu, R. Young, S. Yoshida, T. Liu, T. Meures","submitted_at":"2014-04-21T19:44:28Z","abstract_excerpt":"The Askaryan Radio Array (ARA) is an ultra-high energy ($>10^{17}$ eV) cosmic neutrino detector in phased construction near the South Pole. ARA searches for radio Cherenkov emission from particle cascades induced by neutrino interactions in the ice using radio frequency antennas ($\\sim150-800$ MHz) deployed at a design depth of 200 m in the Antarctic ice. A prototype ARA Testbed station was deployed at $\\sim30$ m depth in the 2010-2011 season and the first three full ARA stations were deployed in the 2011-2012 and 2012-2013 seasons. We present the first neutrino search with ARA using data take"},"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":"1404.5285","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-04-21T19:44:28Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"cf63ceefbbc24ecf6ba97580065f723b080b8e99a709deb4318b6a6ff866ee29","abstract_canon_sha256":"090afca3ecbbc87f89e3d3a63fb33f5b5e922e6b4cd4f8f8520d6a17e0c9d263"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:23:04.539340Z","signature_b64":"abjNTpGrRgBr05KoxtgS+bIYzeCXexWkxVKP3EDt5ECtbGkGyHMSRo8wK12hTab1vxBU7/gVzLvwj8rMguv9Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5269ee729a14d6dd34940f502cabb1947f9d0bcac66f95beea4428df96fd4398","last_reissued_at":"2026-05-18T01:23:04.538902Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:23:04.538902Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"First Constraints on the Ultra-High Energy Neutrino Flux from a Prototype Station of the Askaryan Radio Array","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"A. Connolly, A. Ishihara, A. Karle, A. Laundrie, A. O'Murchadha, ARA Collaboration: P. Allison, A. Shultz, B. Fox, B. Hill, B. Rotter, C. Bora, C.-C. Chen, C. G. Pfendner, C.-J. Li, C. Miki, D. Seckel, D. Z. Besson, E. Hong, G. Nir, G. S. Varner, H. Landsman, H.-Y. Tu, I. Kravchenko, J. Auffenberg, J. J. Beatty, J. Kelley, J. Nam, J. P. Davies, J. Stockham, J. Touart, K. D. Hoffman, K. Hanson, K. Mase, K. Ratzlaff, L.-C. Hu, M. A. DuVernois, M. Richman, M. Stockham, M. Sullivan, M.-Y. Lu, P. Chen, P. Sandstrom, P. W. Gorham, R. Bard, R. J. Nichol, R. Maunu, R. Young, S. Yoshida, T. Liu, T. Meures","submitted_at":"2014-04-21T19:44:28Z","abstract_excerpt":"The Askaryan Radio Array (ARA) is an ultra-high energy ($>10^{17}$ eV) cosmic neutrino detector in phased construction near the South Pole. ARA searches for radio Cherenkov emission from particle cascades induced by neutrino interactions in the ice using radio frequency antennas ($\\sim150-800$ MHz) deployed at a design depth of 200 m in the Antarctic ice. A prototype ARA Testbed station was deployed at $\\sim30$ m depth in the 2010-2011 season and the first three full ARA stations were deployed in the 2011-2012 and 2012-2013 seasons. We present the first neutrino search with ARA using data take"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.5285","kind":"arxiv","version":3},"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":"1404.5285","created_at":"2026-05-18T01:23:04.538966+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.5285v3","created_at":"2026-05-18T01:23:04.538966+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.5285","created_at":"2026-05-18T01:23:04.538966+00:00"},{"alias_kind":"pith_short_12","alias_value":"KJU644U2CTLN","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_16","alias_value":"KJU644U2CTLN2NEU","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_8","alias_value":"KJU644U2","created_at":"2026-05-18T12:28:35.611951+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2512.00660","citing_title":"Particle Astrophysics with High and Ultrahigh Energy Neutrinos","ref_index":172,"is_internal_anchor":true},{"citing_arxiv_id":"2605.04268","citing_title":"Sensitivity of the As-Built Askaryan Radio Array to Ultra-High Energy Neutrinos","ref_index":28,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KJU644U2CTLN2NEUB5ICZK5RSR","json":"https://pith.science/pith/KJU644U2CTLN2NEUB5ICZK5RSR.json","graph_json":"https://pith.science/api/pith-number/KJU644U2CTLN2NEUB5ICZK5RSR/graph.json","events_json":"https://pith.science/api/pith-number/KJU644U2CTLN2NEUB5ICZK5RSR/events.json","paper":"https://pith.science/paper/KJU644U2"},"agent_actions":{"view_html":"https://pith.science/pith/KJU644U2CTLN2NEUB5ICZK5RSR","download_json":"https://pith.science/pith/KJU644U2CTLN2NEUB5ICZK5RSR.json","view_paper":"https://pith.science/paper/KJU644U2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.5285&json=true","fetch_graph":"https://pith.science/api/pith-number/KJU644U2CTLN2NEUB5ICZK5RSR/graph.json","fetch_events":"https://pith.science/api/pith-number/KJU644U2CTLN2NEUB5ICZK5RSR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KJU644U2CTLN2NEUB5ICZK5RSR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KJU644U2CTLN2NEUB5ICZK5RSR/action/storage_attestation","attest_author":"https://pith.science/pith/KJU644U2CTLN2NEUB5ICZK5RSR/action/author_attestation","sign_citation":"https://pith.science/pith/KJU644U2CTLN2NEUB5ICZK5RSR/action/citation_signature","submit_replication":"https://pith.science/pith/KJU644U2CTLN2NEUB5ICZK5RSR/action/replication_record"}},"created_at":"2026-05-18T01:23:04.538966+00:00","updated_at":"2026-05-18T01:23:04.538966+00:00"}