Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/101390
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dc.contributor.authorAartsen, M.en
dc.contributor.authorAckermann, M.en
dc.contributor.authorAdams, J.en
dc.contributor.authorAguilar, J.en
dc.contributor.authorAhlers, M.en
dc.contributor.authorAhrens, M.en
dc.contributor.authorAltmann, D.en
dc.contributor.authorAnderson, T.en
dc.contributor.authorArchinger, M.en
dc.contributor.authorArguelles, C.en
dc.contributor.authorArlen, T.en
dc.contributor.authorAuffenberg, J.en
dc.contributor.authorBai, X.en
dc.contributor.authorBarwick, S.en
dc.contributor.authorBaum, V.en
dc.contributor.authorBay, R.en
dc.contributor.authorBaker, M.en
dc.contributor.authorBeatty, J.en
dc.contributor.authorTjus, J.en
dc.contributor.authorBecker, K.en
dc.contributor.authoret al.en
dc.date.issued2015en
dc.identifier.citationAstrophysical Journal, 2015; 807(1):46-1-46-17en
dc.identifier.issn0004-637Xen
dc.identifier.issn1538-4357en
dc.identifier.urihttp://hdl.handle.net/2440/101390-
dc.description.abstractIn this paper searches for flaring astrophysical neutrino sources and sources with periodic emission with the IceCube neutrino telescope are presented. In contrast to time-integrated searches, where steady emission is assumed, the analyses presented here look for a time-dependent signal of neutrinos using the information from the neutrino arrival times to enhance the discovery potential. A search was performed for correlations between neutrino arrival times and directions, as well as neutrino emission following time-dependent light curves, sporadic emission, or periodicities of candidate sources. These include active galactic nuclei, soft γ-ray repeaters, supernova remnants hosting pulsars, microquasars, and X-ray binaries. The work presented here updates and extends previously published results to a longer period that covers 4 years of data from 2008 April 5 to 2012 May 16, including the first year of operation of the completed 86 string detector. The analyses did not find any significant time-dependent point sources of neutrinos, and the results were used to set upper limits on the neutrino flux from source candidates.en
dc.description.statementofresponsibilityM. G. Aartsen ... G. C. Hill ... S. Robertson ... B. J. Whelan ... et al., IceCube Collaborationen
dc.language.isoenen
dc.publisherIOP Publishingen
dc.rights© 2015. The American Astronomical Society. All rights reserved.en
dc.subjectAstroparticle physics – binaries; general – BL Lacertae objects; general – galaxies; active – neutrinos – X-rays; binariesen
dc.titleSearches for time-dependent neutrino sources with IceCube data from 2008 to 2012en
dc.typeJournal articleen
dc.identifier.rmid0030032289en
dc.identifier.doi10.1088/0004-637X/807/1/46en
dc.identifier.pubid176719-
pubs.library.collectionChemistry and Physics publicationsen
pubs.library.teamDS11en
pubs.verification-statusVerifieden
pubs.publication-statusPublisheden
Appears in Collections:Chemistry and Physics publications

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