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Hokanson-Fasig, B. J. P. Jones, B. J. Whelan, B. Relethford, B. Ty, C. Arg\\\"uelles, C. Bohm, C. De Clercq, C. Finley, C. F. Tung, C. F. Turley, C. Haack, C. H. Wiebusch, C. Kopper, C. P\\'erez de los Heros, C. Raab, C. Rott, C. Spiering, C. Walck, C. Weaver, C. Wendt, D. Altmann, D. Berley, D. Bindig, D. Bose, D. Chirkin, D. F. Cowen, D. Grant, D. Hebecker, D. Heereman, D. J. Koskinen, D. Lennarz, D. L. Xu, D. Pieloth, D. R. Nygren, D. R. Williams, D. Ryckbosch, D. Rysewyk, D. Seckel, D. Soldin, D. Tosi, D. V. Pankova, D. Z. Besson, E. Bernardini, E. Blaufuss, E. Cheung, E. Friedman, E. Jacobi, E. Pinat, E. Resconi, E. Unger, E. Vogel, E. Woolsey, F. Bos, F. Bradascio, F. D. Wandler, F. Halzen, F. Huang, F. Lauber, F. McNally, F. Tenholt, G. Anton, G. Binder, G. C. Hill, G. de Wasseige, G. H. Collin, G. Kohnen, G. Kr\\\"uckl, G. Maggi, G. Merino, G. Moment\\'e, G. M. Spiczak, G. Neer, G. S. Japaridze, G. Te\\v{s}i\\'c, G. T. Przybylski, G. W. Sullivan, G. Yodh, H. Bagherpour, H. Dembinski, H. Dujmovic, H. Kolanoski, H. Niederhausen, H. Pandya, H.-P. Bretz, I. Al Samarai, I. Ansseau, IceCube Collaboration: M. G. Aartsen, I. C. Rea, I. Taboada, J. A. Aguilar, J. Adams, J. A. Pepper, J. Auffenberg, J. Becker Tjus, J. Bourbeau, J. Braun, J. Brostean-Kaiser, J. Casey, J. C. D\\'iaz-V\\'elez, J. Felde, J. Gallagher, J. G. Gonzalez, J. Hignight, J. J. Beatty, J. J. DeLaunay, J. Kim, J. Kiryluk, J. Kunnen, J. L. Kelley, J. L. Lanfranchi, J. L\\\"unemann, J. Madsen, J. M. Conrad, J. Micallef, J. P. A. M. de Andr\\'e, J. P. Barron, J. P. Dumm, J. P. Koschinsky, J. P. Yanez, J. Sandroos, J. Soedingrekso, J. Stachurska, J. Stettner, J. Tatar, J. Vandenbroucke, J. van Santen, J. Werthebach, J. Wood, K. Andeen, K. B. M. Mahn, K. Clark, K. D. de Vries, K. D. Hoffman, K. Filimonov, K. Ghorbani, K. Hanson, K.-H. Becker, K. Helbing, K. Hoshina, K. Hultqvist, K. Jero, K. Krings, K. Mase, K. Meagher, K. Rawlins, K. Satalecka, K. Wiebe, K. Woschnagg, L. Brayeur, L. Classen, L. Gerhardt, L. K\\\"opke, L. Lu, L. R\\\"adel, L. Schumacher, L. Wille, L. Wills, M. Ackermann, M. Ahlers, M. Ahrens, M. B\\\"orner, M. Brenzke, M. Casier, M. Day, M. de With, M. Dunkman, M. Huber, M. H\\\"unnefeld, M. Jeong, M. J. Larson, M. J. Weiss, M. Kauer, M. Kim, M. Kowalski, M. Kroll, M. Labare, M. Lesiak-Bzdak, M. Leuermann, M. Medici, M. Meier, M. Moulai, M. N. Tobin, M. Plum, M. Rameez, M. Relich, M. Richman, M. Rongen, M. Song, M. Stamatikos, M. Sutherland, M. Tselengidou, M. Usner, M. Vehring, M. Vraeghe, M. Wallraff, M. Wolf, M. Zoll, N. Kurahashi, N. L. Strotjohann, N. van Eijndhoven, N. Wandkowsky, O. Botner, P. A. Evenson, P. A. Toale, P. B. Price, P. Desiati, P. Eller, P. Kalaczynski, P. Nakarmi, P. Peiffer, P. Schlunder, Q. R. Liu, R. Bay, R. Cross, R. G. Stokstad, R. Hellauer, R. Hoffmann, R. Koirala, R. Maruyama, R. Maunu, R. Nahnhauer, R. Reimann, R. W. Moore, S. Axani, S. BenZvi, S. Blot, S. B\\\"oser, S. Bron, S. C. Nowicki, S. Coenders, S. De Ridder, S. E. Sanchez Herrera, S. Fahey, S. Flis, S. Hickford, S. In, S. Kopper, S. Kunwar, S. Mancina, S. Miarecki, S. R. Klein, S. Robertson, S. Sarkar, S. Schoenen, S. Sch\\\"oneberg, S. Seunarine, S. Ter-Antonyan, S. Tilav, S. Toscano, S. Vanheule, S. W. Barwick, S. Westerhoff, S. Yoshida, T. Anderson, T. Carver, T. DeYoung, T. Ehrhardt, T. Fuchs, T. Glauch, T. Gl\\\"usenkamp, T. Karg, T. K. Gaisser, T. Kintscher, T. Kittler, T. Kuwabara, T. Menne, T. Meures, T. Montaruli, T. Palczewski, T. Ruhe, T. R. Wood, T. S\\\"alzer, T. Schmidt, T. Stanev, T. Stezelberger, T. Yuan, U. Katz, U. Naumann, V. Baum, V. di Lorenzo, W. Giang, W. Kang, W. Luszczak, W. Rhode, W. Van Driessche, X. Bai, X. W. Xu, Y. Xu, Z. Griffith","submitted_at":"2017-11-22T03:08:55Z","abstract_excerpt":"Neutrinos interact only very weakly, so they are extremely penetrating. However, the theoretical neutrino-nucleon interaction cross section rises with energy such that, at energies above 40 TeV, neutrinos are expected to be absorbed as they pass through the Earth. Experimentally, the cross section has been measured only at the relatively low energies (below 400 GeV) available at neutrino beams from accelerators \\cite{Agashe:2014kda, Formaggio:2013kya}. Here we report the first measurement of neutrino absorption in the Earth, using a sample of 10,784 energetic upward-going neutrino-induced muon"},"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":"1711.08119","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ex","submitted_at":"2017-11-22T03:08:55Z","cross_cats_sorted":["astro-ph.HE","nucl-ex"],"title_canon_sha256":"de50ba297f88d40f45cd0cce4e5423a9fe84d9fea53a03cc2dbbf1157c27aeb1","abstract_canon_sha256":"f1365d2ea0db3544241cc9e8e4dca8625bc534021eeff43d0373d1016b4b3c21"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:28:10.161700Z","signature_b64":"gjNp07evimTkfTXsrzQZh3dZPTjKUsa+amfWVCYHpvsTzlK0vZnUu2H4iObVQl9FLp/xPDs+f/8PVk+5YdYtAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f1dee29f3cc6da9a6e04a0674a6569eabbc62e88cf6aea26bb8374806a0e4fde","last_reissued_at":"2026-05-18T00:28:10.160871Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:28:10.160871Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Measurement of the multi-TeV neutrino cross section with IceCube using Earth absorption","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","nucl-ex"],"primary_cat":"hep-ex","authors_text":"A. Burgman, A. Christov, A. Franckowiak, A. Goldschmidt, A. Hallgren, A. Ishihara, A. Kappes, A. Karle, A. Keivani, A. Kheirandish, A. Kyriacou, A. Obertacke Pollmann, A. Olivas, A. O'Murchadha, A. R. Fazely, A. Sandrock, A. Schneider, A. Stasik, A. Steuer, A. St\\\"o{\\ss}l, A. Terliuk, A. Turcati, A. Wallace, A. Waza, B. Eberhardt, B. Eichmann, B. Hokanson-Fasig, B. J. P. Jones, B. J. Whelan, B. Relethford, B. Ty, C. Arg\\\"uelles, C. Bohm, C. De Clercq, C. Finley, C. F. Tung, C. F. Turley, C. Haack, C. H. Wiebusch, C. Kopper, C. P\\'erez de los Heros, C. Raab, C. Rott, C. Spiering, C. Walck, C. Weaver, C. Wendt, D. Altmann, D. Berley, D. Bindig, D. Bose, D. Chirkin, D. F. Cowen, D. Grant, D. Hebecker, D. Heereman, D. J. Koskinen, D. Lennarz, D. L. Xu, D. Pieloth, D. R. Nygren, D. R. Williams, D. Ryckbosch, D. Rysewyk, D. Seckel, D. Soldin, D. Tosi, D. V. Pankova, D. Z. Besson, E. Bernardini, E. Blaufuss, E. Cheung, E. Friedman, E. Jacobi, E. Pinat, E. Resconi, E. Unger, E. Vogel, E. Woolsey, F. Bos, F. Bradascio, F. D. Wandler, F. Halzen, F. Huang, F. Lauber, F. McNally, F. Tenholt, G. Anton, G. Binder, G. C. Hill, G. de Wasseige, G. H. Collin, G. Kohnen, G. Kr\\\"uckl, G. Maggi, G. Merino, G. Moment\\'e, G. M. Spiczak, G. Neer, G. S. Japaridze, G. Te\\v{s}i\\'c, G. T. Przybylski, G. W. Sullivan, G. Yodh, H. Bagherpour, H. Dembinski, H. Dujmovic, H. Kolanoski, H. Niederhausen, H. Pandya, H.-P. Bretz, I. Al Samarai, I. Ansseau, IceCube Collaboration: M. G. Aartsen, I. C. Rea, I. Taboada, J. A. Aguilar, J. Adams, J. A. Pepper, J. Auffenberg, J. Becker Tjus, J. Bourbeau, J. Braun, J. Brostean-Kaiser, J. Casey, J. C. D\\'iaz-V\\'elez, J. Felde, J. Gallagher, J. G. Gonzalez, J. Hignight, J. J. Beatty, J. J. DeLaunay, J. Kim, J. Kiryluk, J. Kunnen, J. L. Kelley, J. L. Lanfranchi, J. L\\\"unemann, J. Madsen, J. M. Conrad, J. Micallef, J. P. A. M. de Andr\\'e, J. P. Barron, J. P. Dumm, J. P. Koschinsky, J. P. Yanez, J. Sandroos, J. Soedingrekso, J. Stachurska, J. Stettner, J. Tatar, J. Vandenbroucke, J. van Santen, J. Werthebach, J. Wood, K. Andeen, K. B. M. Mahn, K. Clark, K. D. de Vries, K. D. Hoffman, K. Filimonov, K. Ghorbani, K. Hanson, K.-H. Becker, K. Helbing, K. Hoshina, K. Hultqvist, K. Jero, K. Krings, K. Mase, K. Meagher, K. Rawlins, K. Satalecka, K. Wiebe, K. Woschnagg, L. Brayeur, L. Classen, L. Gerhardt, L. K\\\"opke, L. Lu, L. R\\\"adel, L. Schumacher, L. Wille, L. Wills, M. Ackermann, M. Ahlers, M. Ahrens, M. B\\\"orner, M. Brenzke, M. Casier, M. Day, M. de With, M. Dunkman, M. Huber, M. H\\\"unnefeld, M. Jeong, M. J. Larson, M. J. Weiss, M. Kauer, M. Kim, M. Kowalski, M. Kroll, M. Labare, M. Lesiak-Bzdak, M. Leuermann, M. Medici, M. Meier, M. Moulai, M. N. Tobin, M. Plum, M. Rameez, M. Relich, M. Richman, M. Rongen, M. Song, M. Stamatikos, M. Sutherland, M. Tselengidou, M. Usner, M. Vehring, M. Vraeghe, M. Wallraff, M. Wolf, M. Zoll, N. Kurahashi, N. L. Strotjohann, N. van Eijndhoven, N. Wandkowsky, O. Botner, P. A. Evenson, P. A. Toale, P. B. Price, P. Desiati, P. Eller, P. Kalaczynski, P. Nakarmi, P. Peiffer, P. Schlunder, Q. R. Liu, R. Bay, R. Cross, R. G. Stokstad, R. Hellauer, R. Hoffmann, R. Koirala, R. Maruyama, R. Maunu, R. Nahnhauer, R. Reimann, R. W. Moore, S. Axani, S. BenZvi, S. Blot, S. B\\\"oser, S. Bron, S. C. Nowicki, S. Coenders, S. De Ridder, S. E. Sanchez Herrera, S. Fahey, S. Flis, S. Hickford, S. In, S. Kopper, S. Kunwar, S. Mancina, S. Miarecki, S. R. Klein, S. Robertson, S. Sarkar, S. Schoenen, S. Sch\\\"oneberg, S. Seunarine, S. Ter-Antonyan, S. Tilav, S. Toscano, S. Vanheule, S. W. Barwick, S. Westerhoff, S. Yoshida, T. Anderson, T. Carver, T. DeYoung, T. Ehrhardt, T. Fuchs, T. Glauch, T. Gl\\\"usenkamp, T. Karg, T. K. Gaisser, T. Kintscher, T. Kittler, T. Kuwabara, T. Menne, T. Meures, T. Montaruli, T. Palczewski, T. Ruhe, T. R. Wood, T. S\\\"alzer, T. Schmidt, T. Stanev, T. Stezelberger, T. Yuan, U. Katz, U. Naumann, V. Baum, V. di Lorenzo, W. Giang, W. Kang, W. Luszczak, W. Rhode, W. Van Driessche, X. Bai, X. W. Xu, Y. Xu, Z. Griffith","submitted_at":"2017-11-22T03:08:55Z","abstract_excerpt":"Neutrinos interact only very weakly, so they are extremely penetrating. However, the theoretical neutrino-nucleon interaction cross section rises with energy such that, at energies above 40 TeV, neutrinos are expected to be absorbed as they pass through the Earth. Experimentally, the cross section has been measured only at the relatively low energies (below 400 GeV) available at neutrino beams from accelerators \\cite{Agashe:2014kda, Formaggio:2013kya}. 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