{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:HN4V75QEFAAYE74IZFQQDAJQDB","short_pith_number":"pith:HN4V75QE","schema_version":"1.0","canonical_sha256":"3b795ff6042801827f88c961018130187a2a7e5967739687a8f4d7a11a2de331","source":{"kind":"arxiv","id":"1208.2734","version":1},"attestation_state":"computed","paper":{"title":"The MIDAS telescope for microwave detection of ultra-high energy cosmic rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Berlin, A. Ramos de Castro, B. Rouille d'Orfeuil, C. Bonifazi, C. Williams, E. Amaral Soares, E. Mills, E. M. Santos, E. Zas, J. Alvarez-Mu\\~niz, J. F. Genat, J. R. T. de Mello Neto, J. Zhou, L. C. Reyes, M. Bogdan, M. Boh\\'a\\v{c}ov\\'a, M. Monasor, N. Hollon, P. Facal San Luis, P. Privitera, S. Wayne, W. R. Carvalho Jr","submitted_at":"2012-08-14T00:30:40Z","abstract_excerpt":"We present the design, implementation and data taking performance of the MIcrowave Detection of Air Showers (MIDAS) experiment, a large field of view imaging telescope designed to detect microwave radiation from extensive air showers induced by ultra-high energy cosmic rays. This novel technique may bring a tenfold increase in detector duty cycle when compared to the standard fluorescence technique based on detection of ultraviolet photons. The MIDAS telescope consists of a 4.5 m diameter dish with a 53-pixel receiver camera, instrumented with feed horns operating in the commercial extended C-"},"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":"1208.2734","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2012-08-14T00:30:40Z","cross_cats_sorted":[],"title_canon_sha256":"8f0083ec966afea4166bb9f00fda0b1f3abdfb716d8606c4e8cdb25c4c581660","abstract_canon_sha256":"caeb90bc518a5c7d87fbff362680f5f5969b215c49fa308ce999bda5922e33f9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:55:16.242536Z","signature_b64":"lF3oHI1mwkvSWlrigmfkrImQ/aO8Z8E5qoHfd1yRRRRl3KPtqEJ64adGZmFGxw/7watHl5tF5igQUtfcJ5bsBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3b795ff6042801827f88c961018130187a2a7e5967739687a8f4d7a11a2de331","last_reissued_at":"2026-05-18T01:55:16.242099Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:55:16.242099Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The MIDAS telescope for microwave detection of ultra-high energy cosmic rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Berlin, A. Ramos de Castro, B. Rouille d'Orfeuil, C. Bonifazi, C. Williams, E. Amaral Soares, E. Mills, E. M. Santos, E. Zas, J. Alvarez-Mu\\~niz, J. F. Genat, J. R. T. de Mello Neto, J. Zhou, L. C. Reyes, M. Bogdan, M. Boh\\'a\\v{c}ov\\'a, M. Monasor, N. Hollon, P. Facal San Luis, P. Privitera, S. Wayne, W. R. Carvalho Jr","submitted_at":"2012-08-14T00:30:40Z","abstract_excerpt":"We present the design, implementation and data taking performance of the MIcrowave Detection of Air Showers (MIDAS) experiment, a large field of view imaging telescope designed to detect microwave radiation from extensive air showers induced by ultra-high energy cosmic rays. This novel technique may bring a tenfold increase in detector duty cycle when compared to the standard fluorescence technique based on detection of ultraviolet photons. The MIDAS telescope consists of a 4.5 m diameter dish with a 53-pixel receiver camera, instrumented with feed horns operating in the commercial extended C-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1208.2734","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":"1208.2734","created_at":"2026-05-18T01:55:16.242157+00:00"},{"alias_kind":"arxiv_version","alias_value":"1208.2734v1","created_at":"2026-05-18T01:55:16.242157+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1208.2734","created_at":"2026-05-18T01:55:16.242157+00:00"},{"alias_kind":"pith_short_12","alias_value":"HN4V75QEFAAY","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_16","alias_value":"HN4V75QEFAAYE74I","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_8","alias_value":"HN4V75QE","created_at":"2026-05-18T12:27:09.501522+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/HN4V75QEFAAYE74IZFQQDAJQDB","json":"https://pith.science/pith/HN4V75QEFAAYE74IZFQQDAJQDB.json","graph_json":"https://pith.science/api/pith-number/HN4V75QEFAAYE74IZFQQDAJQDB/graph.json","events_json":"https://pith.science/api/pith-number/HN4V75QEFAAYE74IZFQQDAJQDB/events.json","paper":"https://pith.science/paper/HN4V75QE"},"agent_actions":{"view_html":"https://pith.science/pith/HN4V75QEFAAYE74IZFQQDAJQDB","download_json":"https://pith.science/pith/HN4V75QEFAAYE74IZFQQDAJQDB.json","view_paper":"https://pith.science/paper/HN4V75QE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1208.2734&json=true","fetch_graph":"https://pith.science/api/pith-number/HN4V75QEFAAYE74IZFQQDAJQDB/graph.json","fetch_events":"https://pith.science/api/pith-number/HN4V75QEFAAYE74IZFQQDAJQDB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HN4V75QEFAAYE74IZFQQDAJQDB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HN4V75QEFAAYE74IZFQQDAJQDB/action/storage_attestation","attest_author":"https://pith.science/pith/HN4V75QEFAAYE74IZFQQDAJQDB/action/author_attestation","sign_citation":"https://pith.science/pith/HN4V75QEFAAYE74IZFQQDAJQDB/action/citation_signature","submit_replication":"https://pith.science/pith/HN4V75QEFAAYE74IZFQQDAJQDB/action/replication_record"}},"created_at":"2026-05-18T01:55:16.242157+00:00","updated_at":"2026-05-18T01:55:16.242157+00:00"}