Sökning: WFRF:(Silvestri A) > Time-integrated Sea...
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000 | 13250naa a2203553 4500 | |
001 | oai:DiVA.org:uu-152921 | |
003 | SwePub | |
008 | 110503s2011 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-62979 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-1529212 URI |
024 | 7 | a https://doi.org/10.1088/0004-637X/732/1/182 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-629792 URI |
040 | a (SwePub)uud (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Abbasi, R.4 aut |
245 | 1 0 | a Time-integrated Searches for Point-like Sources of Neutrinos with the 40-string IceCube Detector |
264 | 1 | c 2011 |
338 | a print2 rdacarrier | |
500 | a Publikationen har totalt 262 författare, R. Abbasi et al. | |
520 | a We present the results of time-integrated searches for astrophysical neutrino sources in both the northern and southern skies. Data were collected using the partially completed IceCube detector in the 40-string configuration recorded between 2008 April 5 and 2009 May 20, totaling 375.5 days livetime. An unbinned maximum likelihood ratio method is used to search for astrophysical signals. The data sample contains 36,900 events: 14,121 from the northern sky, mostly muons induced by atmospheric neutrinos, and 22,779 from the southern sky, mostly high-energy atmospheric muons. The analysis includes searches for individual point sources and stacked searches for sources in a common class, sometimes including a spatial extent. While this analysis is sensitive to TeV-PeV energy neutrinos in the northern sky, it is primarily sensitive to neutrinos with energy greater than about 1 PeV in the southern sky. No evidence for a signal is found in any of the searches. Limits are set for neutrino fluxes from astrophysical sources over the entire sky and compared to predictions. The sensitivity is at least a factor of two better than previous searches (depending on declination), with 90% confidence level muon neutrino flux upper limits being between E(2)d Phi/dE similar to 2-200 x 10(-12) TeV cm(-2) s(-1) in the northern sky and between 3-700 x 10(-12) TeV cm(-2) s(-1) in the southern sky. The stacked source searches provide the best limits to specific source classes. The full IceCube detector is expected to improve the sensitivity to d Phi/dE proportional to E-2 sources by another factor of two in the first year of operation. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
650 | 7 | a NATURVETENSKAPx Fysikx Subatomär fysik0 (SwePub)103012 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Subatomic Physics0 (SwePub)103012 hsv//eng |
653 | a astroparticle physics | |
653 | a cosmic rays | |
653 | a neutrinos | |
653 | a Physics | |
653 | a Fysik | |
653 | a fysik | |
700 | 1 | a Abdou, Y.4 aut |
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700 | 1 | a Benabderrahmane, M. L.4 aut |
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710 | 2 | a Stockholms universitetb Fysikum4 org |
773 | 0 | t Astrophysical Journalg 732:1, s. 18-q 732:1<18-x 0004-637Xx 1538-4357 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-152921 |
856 | 4 8 | u https://doi.org/10.1088/0004-637X/732/1/18 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-62979 |
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