{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:OVGXU4CFRDK5T4K375FUT33EE5","short_pith_number":"pith:OVGXU4CF","schema_version":"1.0","canonical_sha256":"754d7a704588d5d9f15bff4b49ef642750aa3ed7cea2b24d6bc588b0cf65872d","source":{"kind":"arxiv","id":"1009.1442","version":1},"attestation_state":"computed","paper":{"title":"The first search for extremely-high energy cosmogenic neutrinos with the IceCube Neutrino Observatory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"A. Franckowiak, A. Goldschmidt, A. Gro{\\ss}, A. Hallgren, A. Homeier, A. Ishihara, A. Kappes, A. Karle, A. Olivas, A. Piegsa, A. R. Fazely, A. Rizzo, A. Schukraft, A. Schultes, A. Silvestri, A. Slipak, A. Tamburro, A. Tepe, A. Van Overloop, B. Christy, B. D. Fox, B. Ruzybayev, B. Semburg, B. Voigt, C. Bohm, C. Colnard, C. De Clercq, C. Finley, C. Ha, C. H. Wiebusch, C. P\\'erez de los Heros, C. Rott, C. Roucelle, C. Spiering, C. Walck, C. Wendt, C. Xu, D. Berley, D. Bertrand, D. Chirkin, D. F. Cowen, D. Grant, D. Hubert, D. J. Boersma, D. J. Koskinen, D. Lennarz, D. Pieloth, D. R. Nygren, D. Rutledge, D. R. Williams, D. Ryckbosch, D. Schneider, D. Seckel, D. Tosi, D. Tur\\v{c}an, D. Z. Besson, E. A. Strahler, E. Bernardini, E. Blaufuss, E. Middell, E. Resconi, F. Clevermann, F. Descamps, F. Halzen, F. Kislat, F. Rothmaier, G. C. Hill, G. de Vries-Uiterweerd, G. Kohnen, G. Kroll, G. M. Spiczak, G. S. Japaridze, G. Stephens, G. T. Przybylski, G. Wikstr\\\"om, G. W. Sullivan, G. Yodh, H.-G. Sander, H. Johansson, H. Kolanoski, H. Landsman, H. S. Matis, H. Wissing, IceCube Collaboration: R. Abbasi, I. Taboada, J. A. Aguilar, J. Adams, J. A. Goodman, J. Auffenberg, J. Berdermann, J. Braun, J. C. Davis, J. C. D\\'iaz-V\\'elez, J. Clem, J. Dreyer, J. Eisch, J. Gallagher, J.-H. K\\\"ohne, J. Jacobsen, J. J. Beatty, J. K. Becker, J. Kiryluk, J. L. Bazo Alba, J. L. Kelley, J. L\\\"unemann, J. Madsen, J. Miller, J. M. Joseph, J. P. Dumm, J. Petrovic, J.-P. H\\\"ul{\\ss}, J. Posselt, J. P. Rodrigues, J. Vandenbroucke, J. van Santen, J. W. Nam, K. Andeen, K. Beattie, K. D. Hoffman, K. Filimonov, K. Han, K. Hanson, K.-H. Becker, K. Helbing, K.-H. Kampert, K. Hoshina, K. Hultqvist, K. Kuehn, K. Laihem, K. Mase, K. Meagher, K. Rawlins, K. Schatto, K. Wiebe, K. Woschnagg, L. Bradley, L. Demir\\\"ors, L. Gerhardt, L. Gladstone, L. K\\\"opke, L. Paul, M. Ahlers, M. Baker, M. Bissok, M. Carson, M. Danninger, M. Geisler, M. Gurtner, M. Kowalski, M. Krasberg, M. Labare, M. L. Benabderrahmane, M. Matusik, M. Merck, M. M. Foerster, M. Olivo, M. Prikockis, M. R. Duvoort, M. Ribordy, M. Schunck, M. Stamatikos, M. V. D'Agostino, M. Wallraff, M. Walter, N. Kemming, N. Milke, N. van Eijndhoven, N. Whitehorn, O. Botner, O. Depaepe, O. Engdeg{\\aa}rd, O. Fadiran, O. Schulz, O. Tarasova, P. A. Evenson, P. A. Toale, P. Berghaus, P. B. Price, P. Desiati, P. Herquet, P. Kenny, P. Majumdar, P. M\\'esz\\'aros, P. Nie{\\ss}en, P. O. Hulth, P. Redl, P. Roth, P. Zarzhitsky, Q. Swillens, R. Bay, R. Ehrlich, R. Franke, R. Ganugapati, R. G. Stokstad, R. Lauer, R. Lehmann, R. L. Imlay, R. Maruyama, R. Morse, R. Nahnhauer, R. Porrata, R. W. Ellsworth, R. Wischnewski, S. Bechet, S. B\\\"oser, S. Buitink, S. Cohen, S. Euler, S. Grullon, S. Hickford, S. H. Seo, S. Hussain, S. Knops, S. Lafebre, S. M. Movit, S. Odrowski, S. Panknin, S. R. Klein, S. Sarkar, S. Schlenstedt, S. Seunarine, S. Stoyanov, S. Ter-Antonyan, S. Tilav, S. W. Barwick, S. Westerhoff, S. Yoshida, T. Abu-Zayyad, T. DeYoung, T. Feusels, T. Gl\\\"usenkamp, T. Griesel, T. Karg, T. K. Gaisser, T. Kowarik, T. Krings, T. Kuwabara, T. Meures, T. Montaruli, T. Ruhe, T. Schmidt, T. Stanev, T. Stezelberger, T. Straszheim, T. Waldenmaier, U. Naumann, W. Huelsnitz, W. Rhode, X. Bai, X. W. Xu, Y. Abdou, Y. Sestayo","submitted_at":"2010-09-08T02:34:15Z","abstract_excerpt":"We report on the results of the search for extremely-high energy (EHE) neutrinos with energies above $10^7$ GeV obtained with the partially ($\\sim$30%) constructed IceCube in 2007. From the absence of signal events in the sample of 242.1 days of effective livetime, we derive a 90% C.L. model independent differential upper limit based on the number of signal events per energy decade at $E^2 \\phi_{\\nu_e+\\nu_\\mu+\\nu_\\tau}\\simeq 1.4 \\times 10^{-6}$ GeV cm$^{-2}$ sec$^{-1}$ sr$^{-1}$ for neutrinos in the energy range from $3\\times10^7$ to $3\\times10^9$ GeV."},"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":"1009.1442","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-09-08T02:34:15Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"e28ec54856d9dfb9804ccfe36fdaebe67313ff0915d26516bedb5e4a1cba2a88","abstract_canon_sha256":"a0a95cac9d06bd6f034f8397f96bf90f3269f580fee906faf2d745633282944c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:21:10.748511Z","signature_b64":"UhPqGR28JtJvWSf/wRD2SHVxlPYeoQS39Qn0OHjNBYwjE9ab/+59tNOIAYEWRnUX29H5PNttXJx+u7VaYxQCCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"754d7a704588d5d9f15bff4b49ef642750aa3ed7cea2b24d6bc588b0cf65872d","last_reissued_at":"2026-05-18T04:21:10.747790Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:21:10.747790Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The first search for extremely-high energy cosmogenic neutrinos with the IceCube Neutrino Observatory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"A. Franckowiak, A. Goldschmidt, A. Gro{\\ss}, A. Hallgren, A. Homeier, A. Ishihara, A. Kappes, A. Karle, A. Olivas, A. Piegsa, A. R. Fazely, A. Rizzo, A. Schukraft, A. Schultes, A. Silvestri, A. Slipak, A. Tamburro, A. Tepe, A. Van Overloop, B. Christy, B. D. Fox, B. Ruzybayev, B. Semburg, B. Voigt, C. Bohm, C. Colnard, C. De Clercq, C. Finley, C. Ha, C. H. Wiebusch, C. P\\'erez de los Heros, C. Rott, C. Roucelle, C. Spiering, C. Walck, C. Wendt, C. Xu, D. Berley, D. Bertrand, D. Chirkin, D. F. Cowen, D. Grant, D. Hubert, D. J. Boersma, D. J. Koskinen, D. Lennarz, D. Pieloth, D. R. Nygren, D. Rutledge, D. R. Williams, D. Ryckbosch, D. Schneider, D. Seckel, D. Tosi, D. Tur\\v{c}an, D. Z. Besson, E. A. Strahler, E. Bernardini, E. Blaufuss, E. Middell, E. Resconi, F. Clevermann, F. Descamps, F. Halzen, F. Kislat, F. Rothmaier, G. C. Hill, G. de Vries-Uiterweerd, G. Kohnen, G. Kroll, G. M. Spiczak, G. S. Japaridze, G. Stephens, G. T. Przybylski, G. Wikstr\\\"om, G. W. Sullivan, G. Yodh, H.-G. Sander, H. Johansson, H. Kolanoski, H. Landsman, H. S. Matis, H. Wissing, IceCube Collaboration: R. Abbasi, I. Taboada, J. A. Aguilar, J. Adams, J. A. Goodman, J. Auffenberg, J. Berdermann, J. Braun, J. C. Davis, J. C. D\\'iaz-V\\'elez, J. Clem, J. Dreyer, J. Eisch, J. Gallagher, J.-H. K\\\"ohne, J. Jacobsen, J. J. Beatty, J. K. Becker, J. Kiryluk, J. L. Bazo Alba, J. L. Kelley, J. L\\\"unemann, J. Madsen, J. Miller, J. M. Joseph, J. P. Dumm, J. Petrovic, J.-P. H\\\"ul{\\ss}, J. Posselt, J. P. Rodrigues, J. Vandenbroucke, J. van Santen, J. W. Nam, K. Andeen, K. Beattie, K. D. Hoffman, K. Filimonov, K. Han, K. Hanson, K.-H. Becker, K. Helbing, K.-H. Kampert, K. Hoshina, K. Hultqvist, K. Kuehn, K. Laihem, K. Mase, K. Meagher, K. Rawlins, K. Schatto, K. Wiebe, K. Woschnagg, L. Bradley, L. Demir\\\"ors, L. Gerhardt, L. Gladstone, L. K\\\"opke, L. Paul, M. Ahlers, M. Baker, M. Bissok, M. Carson, M. Danninger, M. Geisler, M. Gurtner, M. Kowalski, M. Krasberg, M. Labare, M. L. Benabderrahmane, M. Matusik, M. Merck, M. M. Foerster, M. Olivo, M. Prikockis, M. R. Duvoort, M. Ribordy, M. Schunck, M. Stamatikos, M. V. D'Agostino, M. Wallraff, M. Walter, N. Kemming, N. Milke, N. van Eijndhoven, N. Whitehorn, O. Botner, O. Depaepe, O. Engdeg{\\aa}rd, O. Fadiran, O. Schulz, O. Tarasova, P. A. Evenson, P. A. Toale, P. Berghaus, P. B. Price, P. Desiati, P. Herquet, P. Kenny, P. Majumdar, P. M\\'esz\\'aros, P. Nie{\\ss}en, P. O. Hulth, P. Redl, P. Roth, P. Zarzhitsky, Q. Swillens, R. Bay, R. Ehrlich, R. Franke, R. Ganugapati, R. G. Stokstad, R. Lauer, R. Lehmann, R. L. Imlay, R. Maruyama, R. Morse, R. Nahnhauer, R. Porrata, R. W. Ellsworth, R. Wischnewski, S. Bechet, S. B\\\"oser, S. Buitink, S. Cohen, S. Euler, S. Grullon, S. Hickford, S. H. Seo, S. Hussain, S. Knops, S. Lafebre, S. M. Movit, S. Odrowski, S. Panknin, S. R. Klein, S. Sarkar, S. Schlenstedt, S. Seunarine, S. Stoyanov, S. Ter-Antonyan, S. Tilav, S. W. Barwick, S. Westerhoff, S. Yoshida, T. Abu-Zayyad, T. DeYoung, T. Feusels, T. Gl\\\"usenkamp, T. Griesel, T. Karg, T. K. Gaisser, T. Kowarik, T. Krings, T. Kuwabara, T. Meures, T. Montaruli, T. Ruhe, T. Schmidt, T. Stanev, T. Stezelberger, T. Straszheim, T. Waldenmaier, U. Naumann, W. Huelsnitz, W. Rhode, X. Bai, X. W. Xu, Y. Abdou, Y. Sestayo","submitted_at":"2010-09-08T02:34:15Z","abstract_excerpt":"We report on the results of the search for extremely-high energy (EHE) neutrinos with energies above $10^7$ GeV obtained with the partially ($\\sim$30%) constructed IceCube in 2007. From the absence of signal events in the sample of 242.1 days of effective livetime, we derive a 90% C.L. model independent differential upper limit based on the number of signal events per energy decade at $E^2 \\phi_{\\nu_e+\\nu_\\mu+\\nu_\\tau}\\simeq 1.4 \\times 10^{-6}$ GeV cm$^{-2}$ sec$^{-1}$ sr$^{-1}$ for neutrinos in the energy range from $3\\times10^7$ to $3\\times10^9$ GeV."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.1442","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":"1009.1442","created_at":"2026-05-18T04:21:10.747916+00:00"},{"alias_kind":"arxiv_version","alias_value":"1009.1442v1","created_at":"2026-05-18T04:21:10.747916+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.1442","created_at":"2026-05-18T04:21:10.747916+00:00"},{"alias_kind":"pith_short_12","alias_value":"OVGXU4CFRDK5","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_16","alias_value":"OVGXU4CFRDK5T4K3","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_8","alias_value":"OVGXU4CF","created_at":"2026-05-18T12:26:12.377268+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/OVGXU4CFRDK5T4K375FUT33EE5","json":"https://pith.science/pith/OVGXU4CFRDK5T4K375FUT33EE5.json","graph_json":"https://pith.science/api/pith-number/OVGXU4CFRDK5T4K375FUT33EE5/graph.json","events_json":"https://pith.science/api/pith-number/OVGXU4CFRDK5T4K375FUT33EE5/events.json","paper":"https://pith.science/paper/OVGXU4CF"},"agent_actions":{"view_html":"https://pith.science/pith/OVGXU4CFRDK5T4K375FUT33EE5","download_json":"https://pith.science/pith/OVGXU4CFRDK5T4K375FUT33EE5.json","view_paper":"https://pith.science/paper/OVGXU4CF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1009.1442&json=true","fetch_graph":"https://pith.science/api/pith-number/OVGXU4CFRDK5T4K375FUT33EE5/graph.json","fetch_events":"https://pith.science/api/pith-number/OVGXU4CFRDK5T4K375FUT33EE5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OVGXU4CFRDK5T4K375FUT33EE5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OVGXU4CFRDK5T4K375FUT33EE5/action/storage_attestation","attest_author":"https://pith.science/pith/OVGXU4CFRDK5T4K375FUT33EE5/action/author_attestation","sign_citation":"https://pith.science/pith/OVGXU4CFRDK5T4K375FUT33EE5/action/citation_signature","submit_replication":"https://pith.science/pith/OVGXU4CFRDK5T4K375FUT33EE5/action/replication_record"}},"created_at":"2026-05-18T04:21:10.747916+00:00","updated_at":"2026-05-18T04:21:10.747916+00:00"}