{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:ARQ4MDS4VQIODEOR6IDJGHL2NV","short_pith_number":"pith:ARQ4MDS4","schema_version":"1.0","canonical_sha256":"0461c60e5cac10e191d1f206931d7a6d5d06ae3eaaff2ac39ca296b8c2a9d347","source":{"kind":"arxiv","id":"2012.07945","version":3},"attestation_state":"computed","paper":{"title":"The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) Observatory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex"],"primary_cat":"astro-ph.IM","authors_text":"A. Anzalone, A. Haungs, A. L. Cummings, A. Neronov, A. N. Otte, A. V. Olinto, C. Guepin, D. Barghini, D. Mand\\'at, D. R. Bergman, D. Winn, E. A. Hays, E. Gazda, E. G. Judd, E. Kuznetsov, E. Parizot, F. Bisconti, F. Cafagna, F. Fenu, F. Oikonomou, F. Sarazin, F. Stecker, G. Filippatos, G. Medina-Tanco, G. Osteria, G. Pr\\'ev\\^ot, H. Miyamoto, I. De Mitri, J. Eser, J. F. Soriano, J. H. Adams, J. Krizmanic, J. McEnery, J. M. Nachtman, J. S. Perkins, J. W. Mitchell, K.-D. Merenda, K. Fang, K. Shinozaki, K. \\v{C}ern\\'y, L. A. Anchordoqui, L. Marcelli, L. Wiencke, L.W. Piotrowski, M. Bagheri, M. Battisti, M. Bustamante, M. Casolino, M. E. Bertaina, M. H. Reno, M. J. Christl, M. Pech, M. Ricci, M. Unger, M. Zotov, O. Romero Matamala, P. F. Bertone, P. Klimov, P. Picozza, P. Reardon, P. Schov\\'anek, R. Aloisio, R. Caruso, R. Diesing, R. Engel, R. M. Young, R. Ulrich, S. S. Meyer, T. M. Venters, T. Paul, V. Kungel, V. Scotti, \\v{S}. Mackovjak, Y. Onel, Y. Takizawa, Z. Plebaniak","submitted_at":"2020-12-14T21:20:46Z","abstract_excerpt":"The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) is designed to accurately observe ultra-high-energy cosmic rays (UHECRs) and cosmic neutrinos from space with sensitivity over the full celestial sky. POEMMA will observe the extensive air showers (EASs) from UHECRs and UHE neutrinos above 20 EeV via air fluorescence. Additionally, POEMMA will observe the Cherenkov signal from upward-moving EASs induced by Earth-interacting tau neutrinos above 20 PeV. The POEMMA spacecraft are designed to quickly re-orientate to follow up transient neutrino sources and obtain unparalleled neutrino flux"},"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":"2012.07945","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2020-12-14T21:20:46Z","cross_cats_sorted":["astro-ph.HE","hep-ex"],"title_canon_sha256":"830a65c9ad8f5f53db5553945b8456b845bb1201c81668327c36e3015464f4a4","abstract_canon_sha256":"64c958766faebe15f94fcf66d4e2b9d4a775401ea2234d1c790202f52cec7c4f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:45:09.867738Z","signature_b64":"eF+Nfa2EJd+a84ovbbK+9nyLB28QqWlu37ZDut+pjAoBFr0LnDdWT2iCJKNHynqheuFiY0OCBiak+39vAgImAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0461c60e5cac10e191d1f206931d7a6d5d06ae3eaaff2ac39ca296b8c2a9d347","last_reissued_at":"2026-07-05T04:45:09.867218Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:45:09.867218Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) Observatory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex"],"primary_cat":"astro-ph.IM","authors_text":"A. Anzalone, A. Haungs, A. L. Cummings, A. Neronov, A. N. Otte, A. V. Olinto, C. Guepin, D. Barghini, D. Mand\\'at, D. R. Bergman, D. Winn, E. A. Hays, E. Gazda, E. G. Judd, E. Kuznetsov, E. Parizot, F. Bisconti, F. Cafagna, F. Fenu, F. Oikonomou, F. Sarazin, F. Stecker, G. Filippatos, G. Medina-Tanco, G. Osteria, G. Pr\\'ev\\^ot, H. Miyamoto, I. De Mitri, J. Eser, J. F. Soriano, J. H. Adams, J. Krizmanic, J. McEnery, J. M. Nachtman, J. S. Perkins, J. W. Mitchell, K.-D. Merenda, K. Fang, K. Shinozaki, K. \\v{C}ern\\'y, L. A. Anchordoqui, L. Marcelli, L. Wiencke, L.W. Piotrowski, M. Bagheri, M. Battisti, M. Bustamante, M. Casolino, M. E. Bertaina, M. H. Reno, M. J. Christl, M. Pech, M. Ricci, M. Unger, M. Zotov, O. Romero Matamala, P. F. Bertone, P. Klimov, P. Picozza, P. Reardon, P. Schov\\'anek, R. Aloisio, R. Caruso, R. Diesing, R. Engel, R. M. Young, R. Ulrich, S. S. Meyer, T. M. Venters, T. Paul, V. Kungel, V. Scotti, \\v{S}. Mackovjak, Y. Onel, Y. Takizawa, Z. Plebaniak","submitted_at":"2020-12-14T21:20:46Z","abstract_excerpt":"The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) is designed to accurately observe ultra-high-energy cosmic rays (UHECRs) and cosmic neutrinos from space with sensitivity over the full celestial sky. POEMMA will observe the extensive air showers (EASs) from UHECRs and UHE neutrinos above 20 EeV via air fluorescence. Additionally, POEMMA will observe the Cherenkov signal from upward-moving EASs induced by Earth-interacting tau neutrinos above 20 PeV. The POEMMA spacecraft are designed to quickly re-orientate to follow up transient neutrino sources and obtain unparalleled neutrino flux"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2012.07945","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2012.07945/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":"2012.07945","created_at":"2026-07-05T04:45:09.867279+00:00"},{"alias_kind":"arxiv_version","alias_value":"2012.07945v3","created_at":"2026-07-05T04:45:09.867279+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2012.07945","created_at":"2026-07-05T04:45:09.867279+00:00"},{"alias_kind":"pith_short_12","alias_value":"ARQ4MDS4VQIO","created_at":"2026-07-05T04:45:09.867279+00:00"},{"alias_kind":"pith_short_16","alias_value":"ARQ4MDS4VQIODEOR","created_at":"2026-07-05T04:45:09.867279+00:00"},{"alias_kind":"pith_short_8","alias_value":"ARQ4MDS4","created_at":"2026-07-05T04:45:09.867279+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2509.09590","citing_title":"Ultra-high energy event KM3-230213A as a cosmogenic neutrino in light of minimal UHECR flux models","ref_index":29,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14409","citing_title":"Astrophysical bounds on the high-energy evolution of neutrino mixing","ref_index":164,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ARQ4MDS4VQIODEOR6IDJGHL2NV","json":"https://pith.science/pith/ARQ4MDS4VQIODEOR6IDJGHL2NV.json","graph_json":"https://pith.science/api/pith-number/ARQ4MDS4VQIODEOR6IDJGHL2NV/graph.json","events_json":"https://pith.science/api/pith-number/ARQ4MDS4VQIODEOR6IDJGHL2NV/events.json","paper":"https://pith.science/paper/ARQ4MDS4"},"agent_actions":{"view_html":"https://pith.science/pith/ARQ4MDS4VQIODEOR6IDJGHL2NV","download_json":"https://pith.science/pith/ARQ4MDS4VQIODEOR6IDJGHL2NV.json","view_paper":"https://pith.science/paper/ARQ4MDS4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2012.07945&json=true","fetch_graph":"https://pith.science/api/pith-number/ARQ4MDS4VQIODEOR6IDJGHL2NV/graph.json","fetch_events":"https://pith.science/api/pith-number/ARQ4MDS4VQIODEOR6IDJGHL2NV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ARQ4MDS4VQIODEOR6IDJGHL2NV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ARQ4MDS4VQIODEOR6IDJGHL2NV/action/storage_attestation","attest_author":"https://pith.science/pith/ARQ4MDS4VQIODEOR6IDJGHL2NV/action/author_attestation","sign_citation":"https://pith.science/pith/ARQ4MDS4VQIODEOR6IDJGHL2NV/action/citation_signature","submit_replication":"https://pith.science/pith/ARQ4MDS4VQIODEOR6IDJGHL2NV/action/replication_record"}},"created_at":"2026-07-05T04:45:09.867279+00:00","updated_at":"2026-07-05T04:45:09.867279+00:00"}