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000207119 005__ 20250730145603.0
000207119 0247_ $$2doi$$a10.1088/0004-637X/796/2/109
000207119 0247_ $$2ISSN$$a0004-637X
000207119 0247_ $$2ISSN$$a0004-637x
000207119 0247_ $$2ISSN$$a1538-4357
000207119 0247_ $$2arXiv$$aarXiv:1406.6757
000207119 0247_ $$2inspire$$ainspire:1303200
000207119 0247_ $$2altmetric$$aaltmetric:2467533
000207119 0247_ $$2openalex$$aopenalex:W2054152824
000207119 037__ $$aPUBDB-2015-01104
000207119 082__ $$a520
000207119 0881_ $$aarXiv:1406.6757
000207119 088__ $$2arXiv$$aarXiv:1406.6757
000207119 1001_ $$0P:(DE-HGF)0$$aAartsen, M. G.$$b0
000207119 245__ $$aSearches for Extended and Point-like Neutrino Sources with Four Years of IceCube Data
000207119 260__ $$aChicago, Ill. [u.a.]$$bUniv.11032$$c2014
000207119 3367_ $$00$$2EndNote$$aJournal Article
000207119 3367_ $$2DRIVER$$aarticle
000207119 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1459942613_28616
000207119 3367_ $$2BibTeX$$aARTICLE
000207119 3367_ $$0PUB:(DE-HGF)15$$2PUB:(DE-HGF)$$aInternal Report$$mintrep
000207119 500__ $$aOA
000207119 520__ $$aWe present results on searches for point-like sources of neutrinos using four years of IceCube data, including the first year of data from the completed 86-string detector. The total livetime of the combined dataset is 1,373 days. For an E$^{-2}$ spectrum the median sensitivity at 90\% C.L. is $\sim 10^{-12}$ TeV$^{-1}$cm$^{-2}$s$^{-1}$ for energies between 1 TeV$-$1 PeV in the northern sky and $\sim 10^{-11}$ TeV$^{-1}$cm$^{-2}$s$^{-1}$ for energies between 100 TeV $-$ 100 PeV in the southern sky. The sensitivity has improved from both the additional year of data and the introduction of improved reconstructions compared to previous publications. In addition, we present the first results from an all-sky search for extended sources of neutrinos. We update results of searches for neutrino emission from stacked catalogs of sources, and test five new catalogs; two of Galactic supernova remnants and three of active galactic nuclei. In all cases, the data are compatible with the background-only hypothesis, and upper limits on the flux of muon neutrinos are reported for the sources considered.We present results on searches for point-like sources of neutrinos using four years of IceCube data, including the first year of data from the completed 86 string detector. The total livetime of the combined data set is 1373 days. For an E (–)(2) spectrum, the observed 90% C.L. flux upper limits are ~10(–)(12) TeV(–)(1) cm(–)(2) s(–)(1) for energies between 1 TeV and 1 PeV in the northern sky and ~10(–)(11) TeV(–)(1) cm(–)(2) s(–)(1) for energies between 100 TeV and 100 PeV in the southern sky. This represents a 40% improvement compared to previous publications, resulting from both the additional year of data and the introduction of improved reconstructions. In addition, we present the first results from an all-sky search for extended sources of neutrinos. We update the results of searches for neutrino emission from stacked catalogs of sources and test five new catalogs, two of Galactic supernova remnants and three of active galactic nuclei. In all cases, the data are compatible with the background-only hypothesis, and upper limits on the flux of muon neutrinos are reported for the sources considered.
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000207119 7001_ $$0P:(DE-H253)PIP1014130$$aAckermann, Markus$$b1
000207119 7001_ $$aAdams, J.$$b2
000207119 7001_ $$0P:(DE-HGF)0$$aAguilar, J. A.$$b3
000207119 7001_ $$aAhlers, M.$$b4
000207119 7001_ $$0P:(DE-HGF)0$$aAhrens, M.$$b5
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000207119 7001_ $$aAnderson, T.$$b7
000207119 7001_ $$aArguelles, C.$$b8
000207119 7001_ $$aArlen, T. C.$$b9
000207119 7001_ $$aAuffenberg, J.$$b10
000207119 7001_ $$aBai, X.$$b11
000207119 7001_ $$aBarwick, S. W.$$b12
000207119 7001_ $$aBaum, V.$$b13
000207119 7001_ $$aBeatty, J. J.$$b14
000207119 7001_ $$0P:(DE-HGF)0$$aBecker Tjus, J. Becker$$b15
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000207119 7001_ $$aBlumenthal, J.$$b27
000207119 7001_ $$aBoersma, D. J.$$b28
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000207119 7001_ $$0P:(DE-HGF)0$$aIceCube Collaboration$$b303$$eCollaboration author
000207119 773__ $$0PERI:(DE-600)1473835-1$$a10.1088/0004-637X/796/2/109$$gVol. 796, no. 2, p. 109 -$$n2$$p109$$tThe @astrophysical journal$$v796$$x1538-4357$$y2014
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