{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,10,8]],"date-time":"2026-10-08T03:07:34Z","timestamp":1791428854005,"version":"4.3.3"},"reference-count":28,"publisher":"American Association for the Advancement of Science (AAAS)","issue":"6161","content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Science"],"published-print":{"date-parts":[[2013,11,22]]},"abstract":"<jats:title>Extraterrestrial Neutrinos<\/jats:title>\n                  <jats:p>\n                    Neutrinos are thought to be produced in astrophysical sources outside our solar system but, up until recently, they had only been observed from one supernova in 1987.\n                    <jats:bold>\n                      Aartsen\n                      <jats:italic>et al.<\/jats:italic>\n                    <\/jats:bold>\n                    (\n                    <jats:related-article xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" ext-link-type=\"doi\" related-article-type=\"in-this-issue\" xlink:href=\"10.1126\/science.1242856\">10.1126\/science.1242856<\/jats:related-article>\n                    ; see the cover) report data obtained between 2010 and 2012 with the IceCube neutrino detector that reveal the presence of a high-energy neutrino flux containing the most energetic neutrinos ever observed, including 28 events at energies between 30 and 1200 TeV. Although the origin of this flux is unknown, the findings are consistent with expectations for a neutrino population with origins outside the solar system.\n                  <\/jats:p>","DOI":"10.1126\/science.1242856","type":"journal-article","created":{"date-parts":[[2013,11,21]],"date-time":"2013-11-21T15:38:32Z","timestamp":1385048312000},"source":"Crossref","is-referenced-by-count":1237,"title":["Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector"],"prefix":"10.1126","volume":"342","author":[{"name":"IceCube Collaboration*","sequence":"first","affiliation":[],"role":[{"vocabulary":"crossref","role":"author"}]}],"member":"221","reference":[{"key":"e_1_3_3_2_2","doi-asserted-by":"publisher","DOI":"10.1016\/j.astropartphys.2006.06.007"},{"key":"e_1_3_3_3_2","doi-asserted-by":"publisher","DOI":"10.1126\/science.1231160"},{"key":"e_1_3_3_4_2","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.111.021103"},{"key":"e_1_3_3_5_2","unstructured":"IceCube Collaboration Observation of the cosmic-ray shadow of the Moon with IceCube arXiv:1305.6811 (2013). http:\/\/arxiv.org\/abs\/1305.6811"},{"key":"e_1_3_3_6_2","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.75.043006"},{"key":"e_1_3_3_7_2","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.78.043005"},{"key":"e_1_3_3_8_2","doi-asserted-by":"publisher","DOI":"10.1016\/j.astropartphys.2012.02.010"},{"key":"e_1_3_3_9_2","doi-asserted-by":"publisher","DOI":"10.1016\/j.nuclphysbps.2013.04.105"},{"key":"e_1_3_3_10_2","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.84.082001"},{"key":"e_1_3_3_11_2","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.110.151105"},{"key":"e_1_3_3_12_2","doi-asserted-by":"publisher","DOI":"10.1007\/BF02509070"},{"key":"e_1_3_3_13_2","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.80.113006"},{"key":"e_1_3_3_14_2","doi-asserted-by":"publisher","DOI":"10.1088\/1126-6708\/2008\/02\/005"},{"key":"e_1_3_3_15_2","doi-asserted-by":"publisher","DOI":"10.1016\/j.astropartphys.2008.02.007"},{"key":"e_1_3_3_16_2","doi-asserted-by":"publisher","DOI":"10.1086\/592213"},{"key":"e_1_3_3_17_2","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.78.2292"},{"key":"e_1_3_3_18_2","doi-asserted-by":"publisher","DOI":"10.1086\/466514"},{"key":"e_1_3_3_19_2","doi-asserted-by":"publisher","DOI":"10.1088\/0004-637X\/745\/1\/45"},{"key":"e_1_3_3_20_2","article-title":"Atmospheric leptons, the search for a prompt component.","author":"Gaisser T. K.","year":"2013","unstructured":"Gaisser T. K., Atmospheric leptons, the search for a prompt component. High Energy Phys. Phenomenol. arXiv:1303.1431 (2013). http:\/\/arxiv.org\/abs\/1303.1431","journal-title":"High Energy Phys. Phenomenol."},{"key":"e_1_3_3_21_2","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.103.221102"},{"key":"e_1_3_3_22_2","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.83.092003"},{"key":"e_1_3_3_23_2","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.79.043009"},{"key":"e_1_3_3_24_2","doi-asserted-by":"publisher","DOI":"10.1016\/j.astropartphys.2013.01.015"},{"key":"e_1_3_3_25_2","doi-asserted-by":"publisher","DOI":"10.1016\/j.nima.2013.01.054"},{"key":"e_1_3_3_26_2","doi-asserted-by":"publisher","DOI":"10.1016\/j.nima.2010.03.102"},{"key":"e_1_3_3_27_2","unstructured":"Heck D. Knapp J. Capdevielle J. Schatz G. Thouw T. CORSIKA: A Monte Carlo Code to Simulate Extensive Air Showers (Forschungszentrum Karlsruhe GmbH Karlsruhe Germany 1998)."},{"key":"e_1_3_3_28_2","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.86.114024"},{"key":"e_1_3_3_29_2","doi-asserted-by":"publisher","DOI":"10.1088\/1126-6708\/2008\/01\/075"}],"container-title":["Science"],"original-title":[],"language":"en","link":[{"URL":"https:\/\/www.science.org\/doi\/pdf\/10.1126\/science.1242856","content-type":"unspecified","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2024,1,10]],"date-time":"2024-01-10T09:33:55Z","timestamp":1704879235000},"score":1,"resource":{"primary":{"URL":"https:\/\/www.science.org\/doi\/10.1126\/science.1242856"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2013,11,22]]},"references-count":28,"journal-issue":{"issue":"6161","published-print":{"date-parts":[[2013,11,22]]}},"alternative-id":["10.1126\/science.1242856"],"URL":"https:\/\/doi.org\/10.1126\/science.1242856","relation":{},"ISSN":["0036-8075","1095-9203"],"issn-type":[{"value":"0036-8075","type":"print"},{"value":"1095-9203","type":"electronic"}],"subject":[],"published":{"date-parts":[[2013,11,22]]},"article-number":"1242856"}}