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All-sky search for time-integrated neutrino emission from astrophysical sources with 7 yr of IceCube data

Abstract:

Since the recent detection of an astrophysical flux of high-energy neutrinos, the question of its origin has not yet fully been answered. Much of what is known about this flux comes from a small event sample of high neutrino purity, good energy resolution, but large angular uncertainties. In searches for point-like sources, on the other hand, the best performance is given by using large statistics and good angular reconstructions. Track-like muon events produced in neutrino interactions satis...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.3847/1538-4357/835/2/151

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Department:
Linacre College
Role:
Author

Contributors

Department:
IceCube Collaboration)
U.S. National Science Foundation More from this funder
University of Wisconsin More from this funder
U.S. Department of Energy More from this funder
Natural Sciences and Engineering Research Council of Canada, More from this funder
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Publisher:
Institute of Physics Publisher's website
Journal:
Astrophysical Journal Journal website
Volume:
835
Issue:
2
Pages:
151
Publication date:
2017-01-24
Acceptance date:
2016-12-06
DOI:
EISSN:
1538-4357
ISSN:
0004-637X
Pubs id:
pubs:646223
URN:
uri:5b4a1606-e596-49f2-893d-f5e01841d545
UUID:
uuid:5b4a1606-e596-49f2-893d-f5e01841d545
Local pid:
pubs:646223

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